The galaxy presents a primarily smooth morphology, with a discernible disk structure. Its shape appears to be somewhere between round and cigar-shaped.  A central bulge is noticeable, exhibiting a brighter luminosity compared to the surrounding disk. There is an absence of clearly defined spiral arms or prominent dust lanes within the galaxy. The light distribution suggests a relatively even stellar population across the galaxy, with no regions exhibiting intense star formation. There are hints of minor disturbances, but it is likely not undergoing any major mergers or strong tidal interactions.  Overall, the galaxy appears to be a relatively undisturbed disk galaxy with a significant bulge component and a fairly homogenous stellar population.
