The galaxy presents as an elliptical or possibly lenticular type. It exhibits a high degree of smoothness, lacking prominent spiral arms or irregular features. The morphology is dominated by a centrally concentrated bulge region, which appears roughly circular in shape. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central bulge. A faint, diffuse halo extends outward from the central region, exhibiting a bluer color, which may be indicative of a lower level of recent star formation activity in the outer regions. There is no visually obvious dust lane or evidence of ongoing mergers or tidal interactions. The overall impression is of a galaxy that is relatively quiescent in terms of current star formation and dynamically relaxed.
