The galaxy exhibits a clear spiral morphology, with tightly wound arms emanating from a bright, yellowish central bulge. The disk component is noticeably larger than the bulge, suggesting a later-type spiral classification. The spiral arms show a granular texture, possibly indicating active star formation regions. The galaxy presents a relatively high degree of rotational symmetry, though with some subtle asymmetries in the arm structure. No prominent bar feature is immediately apparent. The galaxy's overall color profile suggests a population of both older stars in the bulge and younger, bluer stars in the spiral arms, with a slight color gradient noticeable from the center outwards. There is no readily apparent evidence of a major merger or significant tidal disturbances.
