The galaxy presents a somewhat elongated morphology, appearing cigar-shaped. A significant central bulge is evident, exhibiting a bright, concentrated luminosity. Distinct features are observed, possibly indicative of spiral arm structures, however they do not appear well-defined. The galaxy displays a yellowish-red hue, suggesting an older stellar population. There are no clear signs of significant ongoing star formation in the disk. The color gradient indicates a redder core, consistent with an accumulation of older stars. The galaxy may potentially be undergoing or have undergone a merger event. The overall form suggests a late-stage spiral or an elliptical galaxy.
