The galaxy presents as a relatively compact and luminous object. Its overall morphology appears smooth and largely featureless, suggesting a classification towards the elliptical end of the Hubble sequence. While there is some hint of possible disc-like structure, the dominant impression is of a spheroid. The galaxy exhibits a nearly circular profile. No signs of strong tidal interactions or ongoing major mergers are discernible. 

The galaxy appears to be an older stellar population, with a redder color profile. This is indicative of lower current star formation activity and an older stellar population.
