The galaxy presents a generally smooth morphology, with a dominant, concentrated central bulge. There is an indication of a faint, extended disk component, although the resolution limits detailed analysis. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. There are hints of bluer regions in the outer disk, potentially indicating areas of more recent star formation, albeit at a relatively low rate. The galaxy exhibits a somewhat elliptical shape, leaning towards an in-between classification on the roundness spectrum, though it doesn't appear particularly elongated. There are no visually prominent signs of major mergers or significant tidal disturbances in the immediate vicinity, suggesting a relatively undisturbed evolutionary history, though a minor disturbance cannot be ruled out. Overall, the galaxy appears to be an intermediate-mass system with characteristics of both elliptical and spiral galaxies, possibly a lenticular galaxy transitioning from active star formation to a more quiescent state.
