The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. It displays a somewhat elongated, cigar-shaped morphology, suggesting a slight degree of ellipticity. The central region of the galaxy exhibits a yellowish-orange hue, possibly indicative of an older stellar population. A subtle bluish tinge is visible in the outer regions of the galaxy, potentially signaling the presence of some younger, hotter stars. The galaxy shows no signs of strong disturbances, such as tidal tails or obvious asymmetries, indicating that it is not undergoing a major merger event, or has completed the merger process. Overall, the galaxy appears to be a relatively undisturbed system with a dominant spheroidal component.
