The galaxy presents as a centrally concentrated, relatively smooth object with a notable radial intensity gradient. The core region exhibits a bright, almost unresolved luminosity. The overall morphology suggests an elliptical galaxy, potentially of type E0-E3, given its apparently round shape and lack of prominent spiral arms or a distinct disk. The galaxy displays a slight elongation. There is no clear evidence of significant dust lanes or ongoing star formation. Faint, diffuse emission surrounds the central region, gradually fading into the background. There do not appear to be any significant tidal features or distortions indicative of recent major mergers.
