The galaxy presents as a generally smooth, elliptical morphology with a concentrated, bright central bulge. There is minimal apparent disk structure. The overall color profile suggests an older stellar population, with a yellow to orange hue dominating. Indications of recent star formation are weak, based on the lack of prominent blue regions. There is no obvious sign of strong tidal interactions or major mergers, but a slight asymmetry to the outer regions might indicate minor gravitational disturbance. The galaxy appears relatively isolated, though further investigation into surrounding galaxies may reveal some past or ongoing small interactions. The overall structure is quite regular and concentrated.
