The galaxy presents as an elliptical-like structure with a smooth overall appearance. The color profile is dominated by warmer tones, suggestive of an older stellar population. There appears to be some ongoing interaction or a possible merger event occurring. Light distribution seems fairly concentrated, with a higher density towards the center of the galaxy. A slight asymmetry can be observed. The size appears moderate, but given the distance, it seems that the galaxy contains a considerable stellar mass. There is very little evidence of dust lanes or significant spiral arm structures. A faint halo can be seen around the galaxy.
