The galaxy presents as a largely featureless, elliptical-like structure with a concentrated central bulge. The light distribution appears smooth and spheroidal, with a gradual decrease in intensity from the center outwards. It has an overall yellowish hue, suggesting an older stellar population. There are no obvious spiral arm structures or dust lanes visible in the image. The galaxy appears to be relatively isolated, with no obvious signs of recent or ongoing major merger activity, although there is minor asymmetric light distribution surrounding the main body. Its overall morphology indicates a classification towards the early-type end of the Hubble sequence. 
