This galaxy appears to be a spiral galaxy, viewed at a slight angle from face-on. The central bulge is moderately sized and exhibits a smooth, yellowish-white color, suggesting an older stellar population. Winding outwards from the bulge are spiral arms, though they appear somewhat tightly wound. The spiral arms are a bluer color, indicating the presence of younger, hotter stars and active star formation regions. There is no apparent bar structure. No signs of major interaction or merging are visible, although subtle irregularities within the disk may suggest minor past interactions. The overall morphology suggests that the galaxy is in a relatively quiescent state.
