The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a primarily elliptical morphology with a high degree of central luminosity, suggesting a prominent bulge component. The galaxy's light profile appears generally smooth, lacking obvious spiral arm structures or significant dust lanes, but there are subtle features that could suggest the presence of a disk. The color profile indicates a somewhat redder hue, which may be indicative of an older stellar population and/or significant dust obscuration within the galaxy. The overall morphology suggests a galaxy that is either an elliptical galaxy, or perhaps a spiral that is relatively face-on, which limits our ability to observe the spiral structure directly. There is a slight asymmetry to the outer isophotes which may indicate a minor interaction or past merger event, although this is not immediately obvious. There is no visual evidence of a major merger or significant tidal disturbances.
