The galaxy presents as a cigar-shaped, elongated structure, indicating an elliptical morphology or a highly inclined disk galaxy. A distinct central bulge is apparent, exhibiting a concentrated, yellowish-white luminosity, suggesting a population of older, evolved stars. Moving outwards from the bulge, the light gradually fades into a more diffuse halo. The presence of faint bluish-white regions at the edges suggests ongoing, albeit potentially low-level, star formation activity in the outskirts. These regions are not sharply defined, indicating that the star formation is not occurring in large, distinct clusters. There is no evidence of spiral arm structures or a prominent dust lane bisecting the galaxy, further supporting its elliptical nature. The overall smoothness of the light distribution suggests a relatively quiescent galaxy, undisturbed by recent major mergers, though subtle irregularities might suggest minor interactions in the past. The galaxy appears relatively isolated in the field, with no immediate signs of tidal distortions or companion galaxies contributing to its morphology.
