The galaxy presents as a centrally concentrated elliptical-like structure. It appears largely featureless with a smooth luminosity profile, lacking prominent spiral arms or distinct dust lanes. The core region exhibits a yellowish-white hue, suggesting an older stellar population. The galaxy has an estimated effective radius of approximately 4 kpc. The overall color index indicates a red-sequence galaxy, consistent with a relatively quiescent star formation rate. There is no strong visual evidence of tidal interactions or ongoing merging events, though subtle asymmetries may suggest minor past disturbances. The galaxy's shape appears to be somewhere between elliptical and a flattened disk, but is primarily elliptical.
