The galaxy presents a relatively smooth morphology, with a dominant spheroidal component. There is evidence of a faint disk structure viewed nearly edge-on. The central bulge appears prominent and displays a reddish hue, suggesting an older stellar population. Fainter blueish emission is seen in the disk, indicative of ongoing star formation, however it is likely to be low-level. The overall structure shows no strong signs of major mergers or significant tidal disturbances, though subtle asymmetries cannot be ruled out. The galaxy's roundness suggests it is not a highly elongated or cigar-shaped system.
