The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. There appears to be a tidal interaction with a nearby object. There is a noticeable color gradient, transitioning from a more reddish hue in the central regions to a slightly bluer tinge towards the edges. The light distribution suggests a higher concentration of older stellar populations in the core, while younger stars may be forming, or have recently formed, in the outer regions. There are no readily apparent spiral arm structures. The galaxy exhibits signs of disturbance and merging activity in the form of a second, smaller object that may be a satellite galaxy, or the tidal tail of a larger galaxy further away.
