The galaxy presents as a relatively smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, exhibiting a bright core that gradually fades outwards. The overall color appears to be yellowish, suggesting a population of older stars with minimal ongoing star formation. There is no visible evidence of significant dust lanes or recent merger activity that would disrupt the smooth morphology. The galaxy appears isolated, without obvious signs of tidal interactions with neighboring galaxies.
