The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge that emits a significant amount of light. There is a noticeable radial decrease in surface brightness outwards from the core with an apparent lack of distinct features such as spiral arms or dust lanes. The overall color appears to be subtly redder than the surrounding space, suggesting a stellar population dominated by older, redder stars and indicating a low rate of current star formation. The galaxy's shape is closer to being in-between circular and elliptical in appearance. No signs of recent or ongoing merger events are visually evident, the light distribution seems largely undisturbed.
