The galaxy presents as a centrally concentrated object with an overall smooth appearance, lacking strong spiral arm structures or a prominent central bar. The morphology is primarily elliptical or lenticular. There appears to be minimal evidence of ongoing major mergers or significant tidal disturbances, although subtle asymmetries or minor disturbances might be present in the outer regions.

The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward, a faint blueish color becomes more apparent, possibly indicating the presence of younger stars. Star formation seems to be ongoing, although at a relatively modest rate. The galaxy is of considerable mass, and the light is dominated by stars rather than non-stellar activity. The galaxy's shape is more in-between the range of round and cigar shaped.
