The observed galaxy presents as a moderately luminous, lenticular or early-type spiral galaxy, seen at an oblique angle. It exhibits a smooth, centrally concentrated bulge, transitioning to a flattened disk component. The bulge region presents with a yellowish hue, suggestive of an older stellar population. The disk shows a slight bluish tint, particularly on the outer edges, potentially indicating regions of more recent or ongoing star formation. The galaxy's overall morphology lacks any prominent spiral arm structure or significant disturbances, leaning towards a relatively undisturbed system. There is a slight asymmetry in the overall light distribution, suggestive of a possible minor interaction or merger event in the past.
