The galaxy presents a roughly elliptical morphology, characterized by a centrally concentrated luminosity profile. The core exhibits a yellowish hue, which may indicate an older stellar population. The galaxy's outer regions display a bluer tint, possibly indicative of ongoing or recent star formation. There appear to be some slight disturbances in the morphology, perhaps indicating a minor gravitational interaction or internal dynamic activity. There is no definitive spiral structure observed, but the overall appearance suggests the potential for a disk-like component. The galaxy is relatively compact and appears to be moderately massive with a measurable star formation rate.
