The galaxy presents a generally smooth morphology with a slight elongation, appearing somewhat cigar-shaped. The light distribution is concentrated towards the center, suggesting a prominent bulge component. The color gradient indicates a central yellowish or reddish hue, likely associated with an older stellar population, transitioning to bluer colors in the outer regions, which may indicate the presence of younger stars. There is no clear evidence of spiral arms or significant dust lanes, and the galaxy does not appear to be undergoing any major mergers or tidal disturbances. It appears to be a relatively isolated galaxy.
