The galaxy presents a generally smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated, with a gradual decline in surface brightness from the core outwards. The color profile suggests a population dominated by older stars, as indicated by the yellowish-red hue, which could be from the relatively minimal ongoing star formation. There appears to be some minor disturbance visible within the galaxy shape, potentially from a previous interaction, but the galaxy has a fairly round profile. 
