The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. It exhibits a dominant spheroidal component, appearing nearly round in projection. There is subtle color variation across the galaxy, with a warmer, more yellow-orange hue concentrated in the central bulge region and a slightly bluer, diffuse halo extending outwards. The lack of distinct spiral arms or prominent dust lanes suggests a relatively passive or evolved stellar population. There is a potential indication of minor tidal disturbance or a faint plume extending from one side, though the low resolution makes it difficult to confirm the presence of ongoing or recent merger activity. Overall, it appears to be a relatively massive galaxy with a moderate amount of star formation activity.
