The galaxy presents as a somewhat compact and relatively smooth structure. The light distribution suggests a centrally concentrated morphology, possibly an elliptical galaxy, or a spiral galaxy seen face-on with a dominant bulge. There is a slight elongation, but overall the galaxy appears fairly round. The color profile indicates an older stellar population. The galaxy exhibits a reddish-yellow hue, suggestive of evolved stars and a lack of significant ongoing star formation. There is no distinct spiral arm structure or prominent dust lanes visible. Hints of disturbance are present. There are indications of a possible minor interaction with another galaxy or some internal asymmetries, though this is somewhat ambiguous given the resolution. The overall appearance suggests a high-mass galaxy with suppressed star formation.
