The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The overall shape is elongated, approximately cigar-shaped, with the major axis exhibiting a distinct orientation. There is little evidence of spiral arm structure or significant dust lanes. The central region appears significantly brighter and more concentrated than the outer regions. The color profile suggests a population of older stars dominating the overall light emission, as indicated by the reddish hue of the galaxy. There is no clear evidence of ongoing major merging activity. However, there is a slight asymmetry visible which suggests a possible minor disturbance or past interaction. Star formation appears relatively quiescent.
