The galaxy presents as a cigar-shaped form, indicative of an elliptical or lenticular classification. Its light profile appears relatively smooth and homogenous, suggesting a lack of significant dust lanes or prominent spiral arms. The core exhibits a slightly brighter concentration of light, transitioning outwards to a more diffuse halo. Coloration is generally reddish-yellow, which may indicate a population of older stars and limited ongoing star formation. There is a possible indication of tidal disturbance or interaction with other galaxies in the vicinity.
