The galaxy exhibits a somewhat elongated morphology, appearing more disk-like than spheroidal. There is a bright central region, suggestive of a concentrated nucleus. Evident spiral arm structures or prominent dust lanes are not readily discernible. However, a slight asymmetry in the brightness distribution and shape is observed, potentially indicating a past or ongoing interaction. The color profile suggests a mix of stellar populations; a bluer hue in the central area may indicate younger, hotter stars, while the outer regions appear redder, possibly due to older stars or dust obscuration. Faint extensions of the galaxy extend outwards, but are not well defined. A degree of disturbance is present in the overall structure.
