The galaxy presents as an elliptical or lenticular system, exhibiting a centrally concentrated spheroid structure. The light profile is smooth, with no discernible spiral arms or distinct features indicative of active star formation regions such as HII regions or prominent dust lanes. The color gradient suggests an older stellar population, with the core exhibiting a yellowish-orange hue that transitions to a redder, less luminous outer halo. The overall shape is moderately elongated. There is no obvious evidence of tidal disturbances or interaction with other galaxies. The light is fairly smooth, indicating a possible lack of active star formation within the system. Based on these characteristics, this galaxy is likely to be a relatively massive and evolved system.
