The galaxy presents a generally smooth morphology. It appears elliptical, exhibiting a shape somewhere between round and oblong, with a slight preference towards an intermediate shape. There is no strong evidence of spiral arms or a distinct disk structure. The galaxy is centrally concentrated with a bright core that diffuses outwards into an envelope. The color profile suggests a relatively older stellar population. A yellow-orange hue dominates the central region, with a subtle transition to slightly bluer tones in the outer regions. The overall smooth and concentrated light distribution, along with the color profile, indicates that this is a relatively massive system, potentially a lenticular or elliptical galaxy. There is no obvious sign of any major ongoing merger activity, although a subtle, minor disturbance cannot be completely ruled out at this resolution.
