The galaxy appears as a centrally concentrated elliptical or lenticular system with a smooth morphology. It exhibits a near-spherical shape. The central region of the galaxy is a bright yellowish-white, suggesting a significant population of older stars. Fainter, more diffuse greenish light extends outwards from the center, indicating a less concentrated stellar distribution or potentially regions of lower-level ongoing star formation. There is no strong evidence of spiral arms, bars, or any major disturbances due to interactions or mergers, though a slight irregularity in the outer regions hints at a possible minor interaction. Overall, the galaxy exhibits a well-defined, regular structure.
