The galaxy presents as a bright, relatively smooth object. The light distribution is centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The core region exhibits a yellowish hue, possibly indicative of an older stellar population. A small orange feature is visible to the side of the main body of the galaxy. It is possible this is a region of active star formation. The overall shape appears somewhat rounded, but there may be some subtle distortions suggestive of minor gravitational interaction or internal dynamics. There is no clear evidence of a prominent disk structure or spiral arms. There may be a large amount of dust obscuring the galaxy.
