The galaxy presents as a fairly compact object, appearing smooth in texture. The overall color profile is notably redder than blue, implying a potentially older stellar population and/or significant dust obscuration. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor significantly elongated. There is no obvious visual evidence of ongoing major merging activity or strong tidal disturbances. The morphology suggests a possible elliptical galaxy, or a lenticular galaxy viewed at a relatively low inclination. The galaxy is relatively bright, and appears to have a moderate to high mass. The color and smoothness could indicate ongoing, but slow, star formation.
