The galaxy presents as a fairly compact, centrally concentrated object. Its morphology appears smooth, with no distinct spiral arms or bar structures visible. The light profile suggests a spheroidal shape with a gradual decrease in intensity moving outwards from the core. There is a central luminous region which could be indicative of an active galactic nucleus or a dense concentration of older stars. The galaxy appears generally undisturbed, showing no signs of ongoing major mergers or tidal interactions. The overall color suggests a population dominated by older, redder stars. Star formation rates appear to be low based on the color and lack of discernable blue regions. 
