The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, displaying a bright, well-defined core. Moving outward from the core, the light gradually diffuses, forming a more extended halo. A subtle color gradient is visible, with the central regions exhibiting a somewhat redder hue compared to the outer areas, which appear slightly bluer. This may indicate an older stellar population is centrally located within the galaxy, with younger, bluer stars populating the outer regions. There are no apparent spiral arms, rings, or bars present. Additionally, there is no strong evidence of any tidal features, indicating a lack of recent major mergers or interactions.
