The galaxy presents as a moderately sized, elongated structure. Its morphology appears to be that of a lenticular or an edge-on spiral galaxy, given the observed shape. The light distribution is centrally concentrated, with a smooth, diffused appearance. This indicates an older stellar population with relatively little active star formation. The galaxy is subtly elongated, with the major axis being several times longer than the minor axis. There is a suggestion of a central bulge, though it lacks strong definition in this image. The lack of any significant dust lanes or prominent spiral arms reinforces the impression of a system dominated by older stars and a lack of ongoing star formation. There are no obvious signs of recent mergers or major disturbances, and the overall structure appears relatively undisturbed. The color suggests a moderate redshift, consistent with a galaxy at intermediate cosmological distances.
