The galaxy presents as a moderately compact object, elongated along a major axis with an approximate aspect ratio of 3:1. The light distribution is relatively smooth, showing little evidence of strong spiral arm features or prominent dust lanes. The central region appears slightly more concentrated, suggesting the presence of a bulge component, although it is not highly pronounced. The overall color of the galaxy leans towards the redder end of the spectrum, indicating an older stellar population with ongoing, albeit moderate, star formation. There is subtle evidence of minor asymmetry or disturbance in the outer regions, suggesting possible past interactions, though a major merger seems unlikely. The morphology is more akin to a smooth, elongated structure rather than a well-defined disk galaxy, with the shape between round and cigar shaped. 
