The galaxy presents a somewhat elongated morphology, appearing neither perfectly spherical nor highly flattened. A central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population dominating this region. Fainter, bluer regions extend outwards from the central bulge, possibly indicating ongoing, albeit subdued, star formation within a disk-like component. There appears to be some minor disturbance or asymmetry in the outer regions of the galaxy, though it's not overtly indicative of a major ongoing merger event. The overall structure implies a spiral or lenticular classification, leaning towards a more intermediate type given the relative prominence of the bulge and less defined spiral arms. The galaxy demonstrates a moderate mass and luminosity, expected for a system at its estimated distance.
