The galaxy appears as a luminous, concentrated entity. The overall morphology is smooth, without any prominent spiral arm structures or significant dust lanes visible. It displays an elliptical shape with a fairly symmetrical brightness profile. The galaxy core exhibits a bright, concentrated region of light, suggesting a possible active galactic nucleus or a dense stellar population. The color index of the galaxy appears redder in the central core, shifting toward bluer hues in the outer regions. This may indicate an older stellar population with little to no ongoing star formation in the central core. There may be interaction or merging events occurring, indicated by potential tidal disturbances or asymmetric features in the galaxy's outskirts.