The galaxy presents as a centrally concentrated elliptical. The light profile smoothly decreases radially from a bright, compact core. There is no evidence of spiral arms or a well-defined disk structure. The overall shape appears nearly circular, showing a slight elongation. Color gradients are subtle, transitioning from a relatively bluer core to a redder halo, implying a change in stellar populations or dust content. No significant dust lanes or prominent star-forming regions are visible. There is a very faint, diffuse halo surrounding the central region, indicating a low level of current star formation activity or the presence of an older stellar population. No signs of tidal interactions or mergers are apparent in the immediate vicinity of the galaxy.
