The galaxy exhibits a largely smooth morphology with a central, concentrated bulge. The overall shape is somewhat elliptical, displaying an intermediate degree of roundness. There are subtle indications of a disk component, but it is not prominent. The color profile suggests an older stellar population, as indicated by the reddish hue towards the galactic core and the muted blue tones in the outer regions. There is no strong evidence of ongoing major mergers or significant tidal disturbances, though minor irregularities in the outer regions could indicate past interactions. Star formation appears to be relatively low, and concentrated towards the disk component of the galaxy.
