The galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. It exhibits a centrally concentrated luminosity profile, with the light intensity decreasing gradually towards the outer regions. The color is generally yellowish, suggesting an older stellar population with fewer young, hot stars. There is a hint of a faint disk-like structure, however, it is not well defined. No significant signs of active star formation regions or dust lanes are immediately apparent. The overall structure suggests it may be a relatively quiescent galaxy that is in a stage of advanced development with little gas accretion or star formation occurring at the present time. There are no signs of recent or ongoing major mergers, although minor disturbances may be present.
