The galaxy presents as a relatively compact, disk-shaped structure exhibiting a moderate degree of inclination relative to the observer's line of sight. The color profile suggests a dominant population of older stars, particularly within the central bulge, which exhibits a pronounced yellowish hue. The disk component appears fainter and bluer, hinting at regions of ongoing, albeit subdued, star formation. There is no strong indication of distinct spiral arm structure or significant dust lane obscuration. The overall morphology appears relatively smooth, with no signs of major mergers or tidal disturbances. The galaxy displays a moderate luminosity and likely sits within a larger galactic halo.
