The galaxy presents as a somewhat elongated, lenticular or possibly spiral structure, observed at an oblique angle relative to our line of sight. A bright, concentrated central bulge dominates the morphology, exhibiting a yellowish hue indicative of an older stellar population. Fainter, bluish light extends from the central region, suggesting the presence of a disk. The disk appears relatively smooth. There is some evidence of asymmetry in the outer regions, but the system does not appear to be undergoing a major merger. There may be minor tidal features. The observed color gradient, transitioning from yellow in the core to blue in the outer disk, is consistent with a radial gradient in stellar population age and/or dust content. Overall, the galaxy seems to be a relatively massive system with a moderate rate of star formation.
