The galaxy presents as a fairly bright, moderately elliptical object with a noticeable bulge. It appears to be relatively smooth in texture, lacking prominent spiral arm structures or irregular features. The color gradient suggests a possible population of intermediate to old stars, exhibiting a redder hue towards the outer regions. The overall morphology indicates a disk galaxy with a Sersic index suggesting it is between a pure disk and a pure bulge galaxy, which, in combination with the lack of spiral arm structure, suggests it may be a lenticular galaxy viewed at an inclination angle.