The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge exhibiting a yellowish hue. The galaxy's profile appears moderately circular, lacking any distinct elongation or bar structure. There is a subtle disk feature present, contributing to a flattened appearance. The light distribution suggests a well-mixed stellar population. No signs of significant ongoing mergers or tidal disturbances are visible. The galaxy demonstrates a relatively low rate of star formation. The blue fringes are likely evidence of some star formation at the edges of the galaxy.
