The galaxy presents as a primarily smooth, elliptical morphology. Its core exhibits a concentrated, bright luminosity, suggesting a significant density of stars. The surrounding halo gradually fades, lacking defined spiral arm structures. The overall color appears reddish-yellow, indicative of an older stellar population with a lower rate of ongoing star formation, which is consistent with its smooth morphological classification. There is no evidence of significant tidal disturbances or mergers in its immediate vicinity. The galaxy's shape is generally rounded.
