The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The central region exhibits a concentrated luminosity profile, suggesting a significant stellar density, possibly indicative of an aging stellar population. The color appears generally redder, hinting at a population dominated by older, evolved stars with a suppressed rate of active star formation. There is no obvious evidence of prominent spiral arms or a distinct disk-like structure. Minor disturbances may be present, but it is difficult to assess from the image alone whether these are due to interactions.
