The galaxy presents a primarily smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a significant stellar population and/or active galactic nucleus. The light profile appears to fade gradually from the core, indicating an older stellar population. A slight asymmetry is observed, perhaps due to past or ongoing minor gravitational interactions. The overall color is consistent with an evolved stellar population, with a redder tinge observed in one area. It is possible this redder area might be a region of dust obscuration or a separate structure. The morphology suggests a relatively quiescent galaxy, with no strong evidence of active star formation or major mergers in recent history, which is supported by its color profile.
