The galaxy appears to be a somewhat smooth, elliptical-like structure with a bright, concentrated central bulge. The light is primarily distributed in a relatively even manner, though there is a slight elongation. There are no prominent spiral arms or distinct dust lanes visible. The color gradient suggests a population of older stars, with the light skewing toward the redder end of the spectrum. The overall morphology indicates that it is likely a relatively quiescent galaxy with minimal ongoing star formation. There are faint signs of tidal disruption or interactions, suggesting the possibility of a past or ongoing minor merger event. 
