The galaxy exhibits an elliptical morphology, appearing generally smooth in structure with a slight elongation. The central region is characterized by a brighter, more concentrated luminosity, indicative of a spheroidal bulge. The galaxy's color gradient suggests a population of older stars dominating the stellar composition. Faint features or a very subtle disk-like component may be present, but it is not clearly defined. There's no sign of ongoing merging activity or major disturbances to the galaxy's structure. Overall, the galaxy appears to be a relatively isolated, mature system.
