The galaxy presents as a relatively smooth object, with a primarily elliptical morphology. There is a concentration of light toward the center, suggestive of a galactic nucleus. A disk component is faintly visible, though largely indistinct, appearing more like a subtle flattening of the overall spheroidal shape. There is little evidence of spiral arm structures or significant dust lanes within the observed wavelengths.

The color profile indicates moderate star formation, with a slightly bluer hue particularly in the outer regions, pointing towards the presence of younger, hotter stars there compared to the more central, yellower bulge. There is no distinct indication of any ongoing major mergers or significant tidal disturbances. Faint, asymmetric extensions or minor perturbations may be present, suggesting possible minor interactions with smaller satellite galaxies or past merger events. The roundness of the galaxy appears more in between with some slight elongation. 
