The galaxy presents a predominantly smooth appearance, suggesting a likely elliptical morphology. It exhibits a moderate degree of elongation, appearing somewhat cigar-shaped rather than perfectly spherical. The primary light distribution is concentrated towards the center, with a noticeable decrease in intensity moving outwards. The galaxy displays a distinct reddish hue, indicating an older stellar population and potentially lower levels of ongoing star formation. There is a suggestion of a minor disturbance or a possible interaction with a nearby object, though the galaxy does not appear to be undergoing a major merger.
