This galaxy exhibits characteristics of both elliptical and spiral morphologies. It appears to have a significant spheroidal component, indicated by a central bulge of relatively uniform brightness. Faint, diffuse arms may be present, but they lack a tightly wound structure. The overall light distribution suggests that the disk may not be the dominant feature. The galaxy has a smooth overall appearance, but may contain some regions with minor disturbances. The presence of these features could indicate recent interactions or internal processes affecting its morphology. The central region appears slightly brighter and bluer compared to the outer regions, which is suggestive of ongoing or recent star formation activity in the galactic core. The stellar population appears to be a mix of older and younger stars. Dust lanes are not prominently visible.
