The galaxy presents a generally smooth, elliptical morphology. Its light profile is centrally concentrated, with a gradual decline in brightness towards the outer regions. The core region exhibits a yellowish hue, indicative of an older stellar population. There's a very faint suggestion of a disk-like structure but it could be a product of how the galaxy is oriented. There is very little in the way of dust lanes or any other obvious features to note. The shape is somewhat elongated, but appears closer to a rounded shape overall. There's no evidence of any ongoing major merger event, but a very slight asymmetry could be indicative of a minor interaction in its past.
