The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a yellowish-white hue, suggesting a population of older, evolved stars. Moving outwards from the core, the galaxy gradually fades into a dimmer, bluish halo. This halo might indicate the presence of younger, bluer stars, though they appear to be present in a relatively low quantity. The overall light distribution is highly concentrated towards the center, lacking any prominent spiral arm structures or distinct features. The shape is elongated, somewhere in between round and cigar-shaped, possibly indicating an E4-E6 classification on the Hubble sequence. There are no indications of major mergers or significant tidal disturbances. Subtle light irregularities may suggest minor interactions or internal processes occurring within the galaxy, although further spectral data would be needed to confirm this.
