The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile. The light appears relatively smooth, with no distinct spiral arm structures or bar features visible at this resolution. There is a discernible color gradient across the galaxy, transitioning from a yellowish hue in the core to a redder color toward the outer regions. This suggests a radial variation in the stellar populations, with potentially older, redder stars dominating the outskirts and younger, bluer stars more concentrated in the center, or a dustier outer region. There is no strong evidence of ongoing major mergers or significant tidal disturbances; the galaxy appears relatively undisturbed.
