The galaxy presents as a relatively smooth, elliptical-like structure. Its color appears to be generally yellowish, suggesting an older stellar population. It displays a high degree of central concentration, with the luminosity gradually decreasing towards the outer regions. There is a slight elongation to the shape, but it is mostly roundish. There is no visible evidence of significant spiral arms, bar structures, or active star formation regions. Indications suggest the possibility of minor gravitational disturbances.
