The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge, with luminosity decreasing gradually towards the outer regions. There is a subtle color gradient, appearing slightly more blueish in the outer regions of the galaxy and more reddish towards the core, suggesting older stellar populations dominate the central bulge and possibly more recent star formation in the outskirts. No distinct spiral arm structures or prominent dust lanes are apparent, indicating it may be a featureless galaxy. There is no evidence of any recent or ongoing major mergers or significant tidal disturbances. It appears fairly isolated, lacking any close companions that would suggest interactions.
