The galaxy presents as an elliptical morphology. The central region exhibits a concentrated, bright yellowish hue, indicative of an older stellar population. Moving outward from the core, the light gradually diminishes, forming a less defined halo. No distinct spiral arms or dust lanes are visible. The overall structure appears smooth, with a slight deviation from perfect roundness; it leans toward an intermediate elliptical shape. There is no discernible evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, though a very slight asymmetry in the halo suggests a possible minor past interaction. The color gradient from the core outwards suggests some degree of ongoing, albeit low-level, star formation activity within the galaxy, in addition to the dominant older stellar population.
