This galaxy presents as a smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in the core, gradually fading outwards. The galaxy appears elongated, deviating from a perfect circular shape; with a cigar shaped structure. There are no visible spiral arms, prominent dust lanes, or other distinct features associated with spiral galaxies. The color gradient suggests a redder core compared to the outer regions, which may indicate an older stellar population concentrated towards the center. Overall, the galaxy's morphology is suggestive of an early-type galaxy that is a lenticular galaxy, possibly an S0 type. There is no evidence of ongoing major merging or tidal disturbances.
