The galaxy presents a largely smooth morphology, with a highly concentrated central bulge that dominates its overall appearance. The light distribution transitions smoothly from the core outwards, showing a decrease in luminosity with increasing radial distance. The galaxy appears to be nearly circular in projection, with a slight elongation that indicates a mild deviation from perfect symmetry. Its color index indicates a primarily older stellar population. A hint of a disk component may be present but is largely obscured, and minor disturbances are visible in its outer regions, suggesting previous interactions. No prominent spiral arms are visible. There is no evidence of a recent major merger.
