The galaxy presents a smooth, elliptical morphology with a relatively high degree of central concentration. The core region exhibits a yellowish hue, suggestive of an older stellar population dominating the central bulge, indicating that the stars here are not as actively forming as they once were. The outer regions of the galaxy appear less luminous and have a subtle blueish tinge compared to the core, potentially indicating a smaller population of younger, bluer stars in the galactic halo. There does not appear to be any obvious spiral arm structure or distinct dust lanes visible. There are no apparent signs of tidal disturbances or ongoing major mergers visible, though there may be minor interactions present but not observable in this image. The galaxy appears moderately bright.
