The galaxy appears to be a relatively smooth, elliptical-type object with a noticeable reddish hue. The central bulge is prominent and elongated, exhibiting a smooth, diffuse light profile. There's a slight hint of a disk-like structure, but it is not well defined. The galaxy appears to have some form of minor disturbance, possibly an ongoing or past merger event. A distinct redder region is visible near the edge of the galaxy, which may indicate an area of ongoing star formation or dust obscuration. The overall color suggests an older stellar population, with some younger, bluer stars possibly present in the aforementioned redder region. The galaxy is compact, with a moderate size. No spiral arms or other complex structures are readily apparent.
