The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is little to no evidence of spiral arms or a defined disk structure. The light distribution appears relatively uniform across the central region, with a gradual decrease in intensity towards the outer edges. Color gradients suggest a dominant population of older stars, exhibiting a yellowish-red hue, indicative of lower star formation activity. There are indications of possible tidal disturbances or ongoing merging activity with other galaxies, as the morphological classification suggests a generally disturbed system. The image suggests a possible elliptical or lenticular galaxy, potentially undergoing some form of interaction.
