The object appears to be a relatively compact galaxy, exhibiting a roughly elliptical morphology. It displays a bright, concentrated central region, possibly indicating a bulge or active galactic nucleus. The light distribution becomes more diffuse with increasing radius, transitioning into a faint outer halo. There is evidence of bluer color in the central regions, possibly indicating younger stellar populations or ongoing star formation, while the outer regions appear redder, potentially due to older stellar populations. There may be some minor distortions, but the system appears to have a generally undisturbed morphology and does not appear to be involved in any major interactions or mergers.
