The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a prominent, yellowish hue, suggesting a population of older stars. Moving outward from the center, there is a transition to a slightly bluer color, implying the presence of some younger stellar populations within the galactic disk. The overall morphology indicates a low degree of disturbance, with no obvious signs of major mergers or significant tidal interactions. The galaxy appears to be in a relatively quiescent state, with a low star formation rate. The shape is more 'in between', not distinctly round or cigar-shaped. There are no apparent spiral arms or a well-defined disk structure.
