The galaxy presents a predominantly smooth morphology, appearing largely featureless at this resolution. It exhibits a centrally concentrated luminosity profile with a relatively round shape. There are hints of a faint disk-like structure surrounding the central bulge, although distinct spiral arms are not discernible. The color gradient suggests a population of older stars in the central region, indicated by the orange-red hue, while the outer regions exhibit a slightly bluer tint, possibly indicating more recent star formation. The galaxy does not appear to be undergoing any major merging events, although some minor asymmetry or subtle disturbances cannot be ruled out.
