The galaxy presents a slightly elongated morphology. The overall color profile suggests a population dominated by older stars, potentially with a significant spheroidal component. There are some irregularities, suggestive of either a past or ongoing interaction. The main body of the galaxy exhibits a diffuse, yellowish hue, characteristic of an older stellar population. A second, smaller and seemingly more distinct component is visible at a slight offset from the main body. This component has a less defined structure, potentially indicating tidal disruption. There is a faint color gradient. The central region has a slightly brighter, yellower color, while the outer regions appear slightly bluer.
