The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arm structure or prominent dust lanes. Its overall shape is more elliptical than spiral, appearing somewhat elongated but not exceptionally so. The light distribution seems centrally concentrated. The color is generally reddish, which could indicate an older stellar population and a relatively low ongoing star formation rate. There's a suggestion of a possible tidal feature or minor disturbance at the bottom that is reddish in color. The lack of strong blue emission implies a paucity of young, hot stars within the bulk of the galaxy. There is a suggestion that this galaxy could possibly be merging with a smaller galaxy.
