The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that decreases in luminosity moving outward. The galaxy's overall shape is roughly rounded, transitioning towards a slightly elongated, non-cigar shape. No distinct spiral arms or prominent disk-like features are discernible. There is no clear indication of ongoing major mergers or significant tidal disturbances. The galaxy displays a color profile suggesting a population of older stars. The rate of star formation is estimated to be low.
