This galaxy exhibits a predominantly smooth morphology, although some faint features are present that suggest it is not entirely elliptical. There is a noticeable, albeit subtle, disk-like structure. The galaxy's light is concentrated in a central bulge, exhibiting a slightly yellow hue, which may indicate an older stellar population in that region. The outer regions are less concentrated and appear bluer, possibly indicating more recent star formation. There appears to be an interaction with another smaller galaxy to the lower right, showing the early stages of a merging event. The brighter part of the galaxy is estimated to be around 9.2 kpc across. There is evidence of ongoing star formation within this galaxy.
