The galaxy presents a flattened, elongated morphology. It is primarily smooth in appearance, with no readily discernible spiral arms or bar structure. The central region is relatively concentrated, exhibiting a yellowish hue, possibly indicative of an older stellar population. Moving outward from the center, the galaxy's color transitions to a bluer shade, suggesting the presence of younger, hotter stars in the outer regions. This color gradient is subtle but noticeable. Overall, the galaxy's shape is somewhat irregular, appearing more cigar-shaped than perfectly circular. There is no obvious sign of ongoing major mergers or tidal interactions, although minor disturbances can not be ruled out. The galaxy's light profile gradually fades into the background sky, without any sharp edges or distinct features.
