This galaxy presents as a relatively smooth, elliptical-like structure. The core appears highly concentrated with a bright yellowish hue, suggesting an older stellar population dominating the central region. The color gradually fades to a redder tone towards the outer regions of the galaxy. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy exhibits a near-spherical morphology, with only a very slight elongation. No signs of ongoing major mergers or tidal disturbances are immediately evident, suggesting it is likely a relatively undisturbed system. Overall, the galaxy appears to be a relaxed, spheroidal system dominated by an older stellar population with little ongoing star formation.
