The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that dominates its morphology. The light distribution appears to be radially symmetric. The color gradient suggests an older stellar population, with the core appearing more yellow/orange suggesting a high concentration of evolved stars. Faint extensions surrounding the central region indicate the presence of a halo or extended stellar envelope. No prominent spiral arm structures or dust lanes are visible. There may be very minor disturbances in the shape, but there are no signs of ongoing major mergers or tidal interactions are apparent in this image. 
