This galaxy exhibits a distinct lenticular morphology, appearing as a flattened disk with a prominent central bulge. The bulge displays a yellowish hue, suggesting a population of older, cooler stars. The disk, viewed at an oblique angle, reveals a smoother structure with less pronounced spiral arm features. Its bluer color indicates the presence of a younger stellar population and ongoing star formation, however at a low rate. The galaxy displays a moderate degree of elongation, deviating from a perfectly circular shape. There is no strong evidence of a major ongoing merger or significant tidal disturbance, although minor asymmetry may indicate past interactions. Overall, the galaxy appears relatively isolated and undisturbed within its environment.
