The galaxy presents a somewhat elliptical morphology, displaying a predominantly smooth structure. The central region exhibits a concentrated luminosity, appearing yellowish, suggestive of an older stellar population. Moving outwards from the core, there is a transition to a bluer hue, indicating the presence of younger stars, and potentially regions of ongoing star formation. There are hints of a disk structure, albeit weakly defined. There is no obvious evidence of strong tidal disturbances or major mergers based on the image alone, although subtle asymmetries suggest minor interactions might have occurred. The galaxy does not have a strong red color.
