The galaxy presents as a relatively smooth, elongated structure, indicating a likely elliptical morphology. The light distribution suggests a concentrated central bulge fading into a diffuse halo. Its color is generally whitish, possibly indicating a lack of significant ongoing star formation and a population of older stars. The galaxy's shape is cigar-like, with a greater length than width. There are no obvious spiral arm structures or prominent dust lanes visible at this resolution. There is no evidence of strong tidal distortions or nearby companion galaxies suggesting an ongoing major merger, but some minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
