The galaxy appears to be a relatively smooth, centrally concentrated object. The light profile suggests an elliptical morphology, although some slight elongation is present. There is no clear indication of spiral arm structure or a prominent disk component. The color is generally uniform, with a tendency toward slightly bluer hues near the center, indicative of younger stellar populations, and redder colors further away from the center. There appears to be a lack of significant dust lanes or patches, and the galaxy shows a moderate redshift. There is some evidence of minor disturbances of some kind. Overall, the galaxy presents as a moderately massive system with ongoing, but low, star formation.
