The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. There is a gradual decrease in luminosity from the center outwards, suggesting a high degree of symmetry. There is little indication of spiral arms, distinct features, or irregularities in the galaxy's structure. Its color is primarily a yellow-white hue, which may be a suggestion of an older stellar population and decreased levels of on-going star formation activity. The overall shape is somewhat round, but slightly elongated. There are no signs of any significant merging events or tidal disturbances in the immediate vicinity of the galaxy. 
