This galaxy exhibits a clear disk morphology, viewed almost perfectly edge-on. The central bulge appears prominent and somewhat boxy. The bulge has a yellowish-orange hue, suggestive of an older stellar population. The disk is significantly bluer, particularly at the outer edges, likely indicating ongoing or recent star formation. There is a visible dust lane running along the mid-plane of the disk, obscuring some of the light from the bulge. No signs of tidal disturbances or major mergers are apparent, although there is a slight asymmetry to the disk, implying the possibility of a minor interaction in the past, or the presence of internal structures like spiral arms that are difficult to resolve at this distance. The galaxy is relatively compact.
