The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless profile. The central region displays a concentrated luminosity gradient, suggesting a prominent galactic nucleus. The color profile transitions from a yellowish hue at the core to a reddish tint towards the outer edges, possibly indicative of an older stellar population dominating the periphery. There appears to be some minor gravitational disturbance present. There is some evidence of diffuse stellar emission extending outwards.
