The galaxy appears as a slightly elliptical, moderately compact object. It exhibits a smooth, centrally concentrated profile suggesting a dominant bulge component.  The core region is noticeably brighter and exhibits a yellow-white hue, indicative of an older stellar population or dust obscuration.  Surrounding the core, a fainter, bluer halo is observed, exhibiting some irregular structure. This halo likely consists of younger stars and regions of ongoing star formation. Faint wisps or arms are barely discernible extending outward from the central region, hinting at a possible spiral structure, though this feature is not prominent. There may be a very minor interaction or disturbance in the galaxy, but it is difficult to tell. Overall, the galaxy presents as a disk galaxy, possibly an intermediate spiral or a lenticular galaxy with some residual star formation activity.
