The galaxy presents as a generally smooth, elliptical morphology with a central concentration of light. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population. Extending outwards from the core, a more diffuse, bluish component is visible, suggesting the presence of some younger stars. The galaxy appears elongated, with a ratio of the major to minor axis suggesting an classification leaning towards an elliptical galaxy rather than a perfectly circular one. There are no prominent spiral arms, bars, or other obvious features indicative of a disk galaxy. There are no signs of a major merger or strong tidal disturbances; however, a slight asymmetry may indicate a minor gravitational interaction in the past. The overall color profile suggests a galaxy that has largely ceased active star formation, though some ongoing star formation seems to be occurring.
