The galaxy presents as a relatively smooth, elliptical structure. A concentrated, bright core is visible, suggestive of an older stellar population. The overall shape appears to be somewhat elongated, deviating slightly from a perfectly circular morphology. There are faint suggestions of diffuse outer regions, though the transition from the core to the surrounding space seems rather gradual. Hints of color variation exist, with the core exhibiting a slightly redder hue, possibly indicative of dust or older stars, while the outer regions show a subtle bluish tint. No obvious signs of a disk structure, spiral arms, or significant tidal disturbances are apparent, implying a quiescent and relatively undisturbed evolutionary history.
