The galaxy presents as a somewhat elongated structure with a bright, concentrated central bulge, potentially indicating an older stellar population dominating its core. The outer regions of the galaxy appear fainter and more diffuse, with a hint of a disk-like morphology, though the image resolution limits a definitive classification. There is no visible spiral arm structure. The colors suggest a relatively low star formation rate, with redder hues prominent, although some bluer tones exist in the surrounding regions. No signs of recent or ongoing major mergers or significant tidal disturbances are apparent from the observed morphology. Overall, the galaxy appears as an intermediate-mass system with characteristics somewhere between elliptical and spiral types.
