The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is an absence of prominent spiral arms or a well-defined disk, lending it a more spheroid appearance. The light profile gradually fades from the bright core outward.

The color distribution across the galaxy shows some subtle variations. The central bulge exhibits a yellower hue, potentially indicative of an older stellar population. Moving outwards from the center, a slight blue tint can be observed, particularly along the equatorial region. This bluer component suggests the presence of younger, hotter stars, possibly indicating recent or ongoing star formation activity.

The galaxy is elongated and mildly disturbed. There is no evidence of any on-going major merger events.
