The galaxy presents as a system comprised of two distinct components, a central, bright, and smooth elliptical or spheroidal structure, and a less defined, fainter bluish region. The brighter component exhibits a yellowish hue, which suggests an older stellar population. It appears largely devoid of significant dust lanes or substructure. Its smooth appearance also indicates a lack of recent major merger activity. The overall shape appears more circular than elongated.

The fainter region is of a bluer hue, possibly indicating areas of more active or recent star formation. The lower surface brightness suggests a lower stellar density. There are also hints of slight disturbance or minor distortion, this might be from the result of a past merger or tidal interactions, but this is not obvious and cannot be confirmed from the image alone.

The galaxy is of moderate size, suggesting a reasonably massive system.
