The galaxy presents a generally smooth appearance, with a concentration of light toward its central regions. The overall shape is somewhat elliptical, with no obvious spiral arm structure visible at this resolution. It appears moderately luminous, with a color profile that suggests a stellar population dominated by older stars. Indications of a potential merger event are discernible, possibly in an early stage, characterized by a disturbed morphology, with some asymmetry and diffuse features that may indicate tidal interactions. There appears to be only minor disturbances however, and it is possible it is a close interaction with a dwarf galaxy. Star formation appears to be relatively low based on its color.
