The galaxy presents as a slightly elongated, lens-shaped structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus or bulge. The light distribution appears relatively smooth, with a gradual decline in brightness from the core outwards. A faint, disk-like structure or spiral arm remnants may be present but this is difficult to resolve, though it is not completely symmetrical and has slight disturbances. The galaxy displays a yellowish-white color, indicative of an older stellar population. There is faint blue-white scattering near the brighter area, which could suggest some ongoing star formation. There is no clear evidence of a strong tidal interaction, major merger, or significant dust lanes visible in this image.
