The galaxy presents as a flattened elliptical or lenticular morphology, with a smooth, concentrated central bulge. There appears to be a faint disk component, though it is not clearly resolved into spiral arms. The color profile indicates an older stellar population, evidenced by the redder hues. There is a slight asymmetry or minor disturbance in the outer regions of the galaxy, suggesting possible interaction with a companion or recent minor merger event. Star formation appears to be generally low across the galaxy. The overall structure lacks significant dust lanes or prominent star-forming regions.
