The galaxy presents as a singular, fairly uniform object with an elliptical morphology. Its overall color appears to be yellowish-orange, suggesting a stellar population dominated by older, redder stars. There may be an interacting galaxy with an apparent merger occurring, with one object appearing slightly larger than the other. There are no distinct spiral arm structures visible. The galaxy exhibits a smooth appearance, with a high degree of central concentration of light. There is no obvious evidence of active star formation within the visible spectrum. A slight asymmetry could be due to a minor disturbance or tidal interaction but could also be merger related.
