The galaxy presents a generally smooth morphology, with a noticeable lack of distinct spiral arms or a prominent bar structure. The overall shape appears to be somewhat elliptical, elongated along one axis, giving it a slightly cigar-shaped appearance. The light distribution suggests a higher concentration of stars towards the center, which gradually diffuses towards the outer edges. There is evidence of color variation, with the central region exhibiting a yellowish-orange hue, potentially indicating an older stellar population. Fainter greenish tints can be seen in the outer regions which may indicate younger stars, and thus more recent star formation. No major disturbances from interactions or mergers are readily apparent in the visual data. The relatively smooth texture suggests that the galaxy is in a relatively stable state.
