The galaxy presents an overall elliptical morphology, exhibiting a smooth, diffuse light distribution. A subtle color gradient is observed, with the central region displaying a slightly yellowish hue, possibly indicative of an older stellar population, while the outer regions appear bluer, suggesting the presence of younger stars or ongoing star formation. There appears to be a minor disturbance in the morphology on one side of the galaxy, potentially indicative of a past or ongoing interaction or minor merger with another galaxy. The galaxy is moderately compact and exhibits a moderate luminosity.
