The galaxy presents as an elliptical or lenticular-like system with a prominent central bulge. Its shape is elongated, displaying a cigar-like appearance rather than being perfectly spherical. The light distribution is relatively smooth across the galaxy, with a central concentration of luminosity that gradually decreases towards the outer edges. There is an indication of a disk-like structure, though it is not sharply defined. No distinct spiral arms are visible. The galaxy exhibits a subtle color gradient, with the core appearing slightly bluer, suggesting the presence of younger stars, while the outer regions show a redder hue, potentially indicating an older stellar population. There is no apparent evidence of ongoing major mergers or tidal disturbances. The overall morphology suggests a relatively evolved system with a moderate amount of star formation.
