The galaxy presents an elliptical morphology with a smooth light distribution, suggesting an early-type classification. The central region exhibits a concentrated, bright core with a yellow-orange hue, indicating an older stellar population. The galaxy gradually fades outwards, becoming less luminous towards its periphery, with an intermediate roundness. There is a slight indication of a minor disturbance, with a small irregular and less concentrated region of light visible on one side of the main body, that could suggest a very minor tidal interaction or merger. The overall color profile leans towards the redder end of the spectrum, consistent with a relatively quiescent galaxy with low ongoing star formation. The galaxy appears relatively isolated, without any strong signs of major mergers or significant morphological distortions beyond the minor disturbance.
