The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. Its shape appears largely spheroidal, closely resembling an elliptical galaxy, with a round appearance. There's a noticeable color gradient, transitioning from a brighter, yellowish core to a fainter, redder outer region.  No prominent spiral arms or strong tidal features are visually apparent, suggesting relative dynamical stability. The galaxy does not appear to be undergoing a major merging event, although it shows some signs of minor disturbances. The colors suggest a population of older stars, though there may be some on-going, low-level star formation activity.
