The galaxy presents an elliptical morphology with a smooth light distribution, showing no apparent spiral arm structure or prominent dust lanes. The galaxy exhibits a centrally concentrated luminosity profile, with the highest intensity observed at its core, gradually decreasing outwards. The color appears primarily red, indicative of an older stellar population, with minimal evidence of recent star formation. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances. The overall shape suggests a relatively high degree of symmetry, with a roundish form, indicating that it is likely a relaxed system.
