The galaxy presents a generally smooth appearance, with a centrally concentrated bulge exhibiting a reddish hue. Surrounding this central region is a less defined, bluer disk or halo, indicating ongoing or recent star formation. The overall shape leans toward elliptical, though some deviation from perfect roundness is apparent. There is no clear evidence of major mergers or significant tidal disturbances in the immediate vicinity, although subtle asymmetries suggest potential minor interactions or internal processes affecting the galaxy's structure.
