The galaxy exhibits a generally smooth morphology, with a slight elongation suggesting a flattened spheroidal shape. There is a central, bright concentration of light, possibly indicating a bulge or active galactic nucleus. Fainter, less defined extensions appear on either side of the central region, possibly indicative of a disk structure or tidal arms, though no spiral structure is readily apparent. The colour profile appears to be dominated by redder wavelengths, with the central region being more intensely red-orange. This suggests a population of older stars, with lower rates of star formation. The lack of distinct features implies that the galaxy is likely an early-type galaxy. However, there also may be a merger happening here, as the structure seems disturbed.
