The galaxy presents as a relatively face-on spiral galaxy, exhibiting a well-defined disk structure. The disk shows evidence of spiral arms, with two major arms prominently visible. These arms appear somewhat tightly wound, wrapping around the central bulge of the galaxy. There is a suggestion of a bar-like structure bisecting the central bulge. The bulge itself appears moderately sized and exhibits a yellowish color, possibly indicating an older stellar population. Star formation is apparent within the spiral arms, indicated by the bluer color. However, the specific star formation rate is somewhat low. The galaxy does not appear to be undergoing any major mergers or significant disturbances.
