The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless profile. Its shape appears somewhat elongated, tending towards a cigar-like form rather than a perfectly spherical distribution. The light distribution is concentrated centrally, diminishing gradually outward, lacking any distinct spiral arms or prominent disk structures. Color gradients are subtle, suggesting a population of older stars, with a generally yellowish hue, especially concentrated toward the center. There may be evidence of minor tidal disturbances or interactions; however, these are not prominently disruptive to the overall structure of the galaxy. The system does not show any prominent dust lanes, and the star formation rate is likely low. It appears to be a fairly massive galaxy, with no indications of a recent major merger.
