The galaxy presents as a luminous, elliptical morphology, displaying a smooth and relatively featureless structure. It exhibits a high degree of roundness. The color profile leans towards the redder end of the spectrum, suggesting an older stellar population and a relatively low rate of star formation. There is no apparent evidence of strong spiral arms, prominent dust lanes, or a distinct central bar. There are no signs of any major merging activity or significant tidal disturbances. The galaxy appears isolated in its immediate environment.
