The galaxy presents as a relatively compact, elliptical-like system, exhibiting a smooth, largely featureless morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The overall color appears yellowish, suggesting a stellar population dominated by older, redder stars and a low rate of ongoing star formation. There is little evidence of spiral arm structure, dust lanes, or prominent star-forming regions. No significant tidal features or signs of major mergers with other galaxies are observed. Subtle asymmetries or minor disturbances cannot be entirely ruled out. The galaxy appears to be relatively isolated. The light distribution suggests a round shape for the galaxy.
