The galaxy presents an elliptical morphology, characterized by a relatively smooth and concentrated distribution of light. The core region exhibits a brighter, more intensely illuminated zone, suggesting a higher concentration of stars. The overall color profile appears to be predominantly yellow-reddish, possibly indicative of an older stellar population, with diminished rates of active star formation. A slight elongation is observed in the shape, suggesting a deviation from perfect sphericity. There appears to be a lack of prominent spiral arms or significant dust lanes. The galaxy appears relatively isolated, without obvious signs of ongoing major merger events or tidal disturbances.
