The galaxy presents a generally smooth and rounded morphology, with a noticeable concentration of light towards the center. The overall color is yellowish-orange, suggesting a stellar population dominated by older, redder stars. There is little to no visible evidence of spiral arms or a prominent disk structure. No signs of active star formation regions or significant dust lanes are apparent, although the image resolution is limited. The galaxy shows no obvious signs of major mergers or tidal disturbances, and its symmetric form points to a relatively settled dynamical state.
