The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. It exhibits a yellowish-red hue, indicative of a stellar population dominated by older, redder stars and/or significant dust obscuration. There is no clear evidence of spiral arms or a bar structure. The galaxy displays a high degree of roundness. There is no apparent major disturbance due to merging activity. There is a lack of blue light indicative of little to no active star formation. 
