This galaxy presents as a relatively compact object. It exhibits a central bulge with a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge is a bluer, less concentrated disc-like structure. The blue color indicates the presence of younger, hotter stars, potentially regions of ongoing or recent star formation. There may be some minor asymmetries or disturbances in the outer regions of the disc, hinting at possible interactions or mergers in its past. The galaxy is neither completely smooth nor clearly defined as a spiral or elliptical, appearing to be somewhere in between. Overall, it seems to be an intermediate-mass galaxy with a mix of stellar populations.
