The galaxy exhibits a moderately defined disk structure. Its visual morphology suggests a classification leaning toward a spiral or possibly a lenticular type. There appears to be some evidence of irregular features, although the resolution limits detailed analysis. Color gradients are subtle, but a slight bluer hue towards the outer regions suggests ongoing star formation, while the central area appears redder, indicating an older stellar population. There are subtle asymmetries in the light distribution. The overall appearance suggests the galaxy might have experienced a minor interaction in its past, although no major tidal features are apparent.
