The galaxy presents a predominantly smooth morphology with a notable lack of prominent spiral arms or bar structures. Its overall shape is elongated, appearing somewhat cigar-shaped. The central region exhibits a concentrated luminosity, suggesting the presence of a significant galactic bulge. Color gradients are subtle, with a yellowish-white hue dominating the core, potentially indicative of an older stellar population. The outer regions appear fainter and slightly bluer, hinting at the possibility of ongoing, though relatively low, star formation activity in the disk. There is no apparent evidence of a major merger event or tidal disturbances; however, some slight asymmetry in the outer regions could suggest minor gravitational interactions. Overall, the galaxy appears to be a relatively evolved system.
