The galaxy presents a moderately smooth, lenticular morphology. The light distribution indicates a flattened spheroid shape, possibly an elliptical galaxy transitioning to a spiral. The central bulge region exhibits a concentrated, intense yellowish hue, indicative of an older stellar population. Fainter and somewhat diffuse disk-like structure extends from the core along a moderately elongated axis. There may be a merging companion or tidal disturbance present. The disturbance is likely causing a bluer color in the galaxy, suggesting possible star formation. A secondary, smaller feature located close to the main galaxy body is suggestive of an ongoing or recent interaction, potentially influencing the overall morphology.
