The galaxy presents as a spiral with a relatively bright, concentrated central bulge. The disk component appears well-defined but not perfectly face-on, exhibiting a slight tilt relative to the observer's line of sight.

Spiral arms are clearly visible, appearing somewhat tightly wound around the central bulge. They exhibit a mottled texture, suggesting active star formation regions interspersed within the spiral structure. A bar structure is evident in the central region, bisecting the bulge and influencing the morphology of the inner spiral arms. 

The galaxy exhibits a color gradient, with the central bulge appearing more yellowish, indicating a population of older stars, while the spiral arms show a bluer tint, consistent with younger, hotter stars forming within gas and dust clouds. There is no evidence of any major mergers or significant tidal disturbances from neighboring galaxies.
