The galaxy presents as a generally smooth, elliptical-like structure. The central bulge appears quite prominent and relatively bright, gradually fading into the surrounding disk. This light gradient suggests a concentration of older stellar populations towards the core, characteristic of evolved galaxies.

The overall color profile tends towards the redder end of the spectrum, indicating a likely paucity of ongoing star formation. There is only a vague hint of spiral arm structure or patchy star-forming regions within the disk, which, if present, are quite subdued. The galaxy appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions.
