The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population with a relative deficiency of ongoing star formation. The overall roundness of the galaxy is notable, with minimal visible deviation from a spheroidal shape. There are no prominent spiral arms or bars discernible. Evidence of recent or ongoing major mergers or significant tidal disturbances is absent. A slight color gradient is observed, with the core appearing more yellow than the outer regions which trend towards redder hues. This could potentially suggest some level of differential stellar population distribution within the galaxy. The object has an approximate half light radius of 6.6 kpc. The luminosity of this galaxy is high.
