The galaxy presents as a central, moderately luminous object. Its overall morphology appears largely smooth and somewhat amorphous, lacking a clearly defined spiral structure or prominent central bulge. The light distribution seems relatively even, though there are some concentrations of luminosity, with a potential slight elongation or tidal tail possibly indicating minor disturbances or interaction. Coloration is predominantly reddish, suggesting an older stellar population, but some regions exhibit a bluer hue, indicating pockets of more recent star formation. The periphery of the galaxy appears diffuse, without sharp boundaries. The presence of some uneven light distribution may potentially indicate recent merger activity or tidal interactions, though the features are not decisively distinct. 
