The galaxy presents as a generally smooth, elliptical morphology, appearing quite rounded in shape. There is a primary, dominant central bulge that exhibits a concentrated luminosity gradient. A faint, diffuse halo seems to surround the central region, though its boundaries are not sharply defined, suggesting a gradual decrease in stellar density outwards.  Color gradients are subtle, with a slightly redder hue towards the core.  There is some evidence of a minor disturbance in the galaxy's structure and it is possible that there are some other galactic objects in close proximity. Despite the subtle disturbance, the galaxy displays an overall relaxed appearance, characteristic of evolved systems. Star formation rate appears to be low.
