The galaxy presents as an elliptical morphology, appearing mostly smooth and with a concentrated central bulge. The light profile suggests a centrally dominant stellar population, exhibiting a yellow/orange hue, indicative of older stars. There is little evidence of spiral arm structure or significant dust lanes. There appears to be a slight deviation from perfect sphericity, leaning towards a more intermediate, oval shape. No significant merging or tidal disturbances are apparent from its structure; it appears as an isolated system. Based on its colour and morphology, this galaxy is likely a massive system with little recent star formation.
