The galaxy presents as a somewhat symmetrical, elliptical-like structure. It exhibits a smooth morphology with a bright central bulge, potentially indicative of an older stellar population. The color gradient shifts from a yellowish-white core to a subtly bluer outer region, suggesting some degree of ongoing star formation, although limited. There's no clear evidence of spiral arms, a prominent disk structure, or major disturbances suggestive of a recent merger event, though minor irregularities are noted. Overall, it has a generally isolated appearance, showing no signs of strong tidal interactions with any neighboring galaxies.
