The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless light distribution. Its shape is close to round, with a slight elongation discernible along one axis. The color profile indicates an older stellar population, with a yellowish-red hue dominating the galaxy's core and outer regions. There is little evidence of distinct spiral arm structures or significant dust lanes. Subtle color variations might suggest minor variations in stellar population density or metallicity across the galaxy's body, but high resolution observations would be required to confirm this. There does not appear to be any significant mergers or tidal disturbances impacting the galaxy's overall form.
