The galaxy presents a primarily smooth morphology, with a high degree of central concentration. Its shape tends towards round. A slight elongation is present along one axis, but the overall structure is not significantly distorted. A central bulge region appears bright and yellowish, indicating a population of older stars. Surrounding the bulge, a fainter, bluer halo is visible, possibly indicative of some ongoing star formation. No prominent spiral arms or bar features are immediately apparent. There may be evidence of minor tidal disturbances or interactions. Based on its properties, it appears to be a relatively massive system, likely a lenticular or early-type spiral galaxy.
