The galaxy appears to be an elliptical type, with a dominant smooth, spheroidal component. A slight elongation is present, indicating a possible deviation from perfect sphericity. The central region exhibits a brighter, more concentrated luminosity profile suggestive of a nucleus or core. A faint, redder extension is visible on one side of the galaxy, possibly a tidal feature or a region of enhanced dust extinction and star formation, which could suggest a minor interaction. Overall, the galaxy appears to be relatively undisturbed.
