The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a high degree of luminosity, appearing as a concentrated source of light. There is a subtle color gradient visible, transitioning from a yellow-white center to a redder hue in the outer regions. The shape is largely rounded, displaying no prominent features indicative of spiral arms or significant disturbances, nor signs of a recent merger. The galaxy is slightly elongated. The observed color suggests a stellar population dominated by older, redder stars. The apparent lack of distinct features implies a low ongoing star formation rate. The galaxy shows no indications of being actively involved in a major interaction or merging event.
