This galaxy appears to be a relatively small, well-defined system at a moderate redshift. It exhibits a predominantly smooth morphology, with an absence of obvious spiral arms or strong bar features. The light distribution suggests a central bulge or core region, surrounded by a more diffuse halo. There is a slight elongation to the object's shape, but it is mostly rounded. The color index indicates a population of primarily older stars and a low rate of ongoing star formation. There is a minor indication of disruption within the system, suggesting past minor disturbances, with no clear signs of a major merger. The object lacks distinct tidal tails or bridges.
