The galaxy presents as a smooth, elliptical form, with a high degree of central concentration. There is minimal evidence of spiral arm structure. The color gradient suggests an older stellar population. The galaxy appears slightly elongated, possibly indicative of an E4-E6 morphological classification on the Hubble sequence. There is a slight bluing of the galaxy towards its outer regions, potentially indicating lower levels of ongoing star formation. No indications of merging or tidal disturbance are evident.
