The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core appears to be dominated by older stellar populations, emitting primarily in the redder wavelengths, indicative of an evolved stellar population. Moving outwards from the core, there's a gradual decrease in luminosity. The halo region exhibits a subtle bluish tint, which could indicate the presence of younger, hotter stars, and potentially some ongoing, albeit limited, star formation. The galaxy displays a degree of elongation; it is more 'in between' and 'cigar shaped' than round. The galaxy does not seem to be interacting or merging with any other galaxies or objects. There are no apparent tidal tails or distorted structures. The galaxy exhibits no significant features or structures besides the smooth luminosity profile.
