The galaxy presents a generally elongated, cigar-shaped morphology. A central bulge appears prominent, exhibiting a yellowish hue, possibly indicative of an older stellar population. Extending outwards from the bulge, a faint disk is observed. It is not possible to confidently state whether there are spiral arms, but the outer regions of the galaxy are bluish in color, which could be explained by the presence of younger, bluer stars. There appear to be no major disturbances or mergers. The overall impression is of a galaxy with a smooth appearance, where the bulge is the dominant feature.
