The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type. There's little evidence of spiral arm structure or prominent dust lanes. The light distribution suggests a diffuse halo surrounding a brighter core, hinting at a substantial stellar population. Its overall shape appears somewhat elongated, but it does not display extreme deviation from circularity. There is a slight suggestion of asymmetry in its outer regions, possibly indicating a past minor interaction or merger. The galaxy displays a moderately red color, indicative of an older stellar population and a reduced rate of ongoing star formation.
