The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology with a high degree of central concentration. The light distribution suggests a spheroid shape, elongated along one axis. There is little evidence of spiral arms or a prominent disk structure. The color appears relatively uniform throughout the galaxy, trending towards yellow-red, possibly indicating a population of older stars. Star formation is occurring at a low rate. No significant tidal disturbances or signs of ongoing mergers with other galaxies are detected.
