The galaxy presents as an elliptical morphology, displaying a smooth, concentrated light profile that gradually fades into the background sky. The core exhibits a yellow-white hue, suggestive of an older stellar population dominating the central region. Progressing outward from the core, the color subtly shifts towards a redder tone, possibly indicating the presence of a slightly younger, but still relatively aged, stellar population within the galaxy's envelope. There's no discernible spiral structure or prominent dust lanes visible. The galaxy appears undisturbed, showing no obvious signs of ongoing or recent major mergers. The overall shape can be described as moderately elongated, falling somewhere in between round and cigar-shaped, with no strong distortions apparent. The galaxy's smooth appearance and color profile suggest a relatively low current rate of star formation.