The galaxy presents an elongated, cigar-shaped morphology, characteristic of an elliptical galaxy viewed at an angle, but could also possibly be a lenticular galaxy. The light distribution appears smooth with a high degree of central concentration that diminishes outwards, with no strong evidence of spiral arms or distinct features. The core region exhibits a yellowish-white hue, suggesting an older stellar population dominated by evolved stars. The outer regions of the galaxy show a subtle transition to a bluer tint. The light distribution is quite smooth, and there are no prominent dust lanes visible. No obvious signs of recent or ongoing merger events are apparent within the immediate vicinity of the galaxy. The overall appearance suggests a relatively quiescent galaxy with a moderate stellar mass, and a subdued rate of star formation.
