The galaxy presents as a relatively smooth, centrally concentrated object. The light is significantly concentrated in the central region, with a noticeable radial decrease in surface brightness towards the outer edges. The morphology is generally elliptical. There is a slight deviation from a perfectly circular profile; it appears somewhat elongated, though not dramatically so. There are indications of minor disturbances within the galactic structure, but the overall impression is that the system is relatively relaxed. The color profile exhibits some variation, with the central region appearing more yellow, gradually shifting to a slightly redder hue in the outer regions. There is a chance of some degree of ongoing or recent merger activity.
