The galaxy presents as a largely featureless, elliptical morphology. The central bulge region exhibits a high concentration of light, appearing yellowish-white in color, indicative of an older stellar population. There is a slight elongation of the galaxy's overall shape, transitioning from round to a cigar-shaped appearance. The disk component is not clearly visible, suggesting it is either absent or observed at an angle that obscures its features. Faint traces of what might be spiral arm structures exist, but it is difficult to identify. No signs of any recent or major merging events, disturbances, or close companion galaxies are immediately obvious in this image. There are no obvious dust lanes or prominent regions of active star formation visible. The galaxy seems relatively isolated and undisturbed.
