The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification. It exhibits an overall circular appearance with high degree of central concentration. The galaxy shows evidence of some internal structure, with a possible disk like feature embedded within the main body. The light profile appears relatively uniform across the galaxy, with some variations indicating areas of slightly enhanced emission. There is a hint of minor gravitational disturbance or interaction occurring, seen in the fuzziness of the galaxy. The galaxy possesses a redder color, possibly indicative of an older stellar population with suppressed star formation.
