The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile suggests a population of older stars, exhibiting a yellowish-red hue. There is little evidence of spiral arms or significant dust lanes, implying a lack of ongoing major star formation. The galaxy displays a fairly round morphology, with no significant tidal disturbances or signs of a recent major merger event, suggesting it is a relatively relaxed system. 
