The galaxy appears as a relatively compact, luminous object, with an apparent elliptical morphology. The core exhibits a notably bright concentration of light, which smoothly declines in intensity moving outward from the central region. The color profile indicates a yellow-red hue. The galaxy appears to be involved in a potential interaction. The shape is mostly round, but there are some irregularities and/or disturbances in the outer regions that might suggest a minor disturbance or a merger event in the distant past. Although the image is rather compact, the light distribution seems fairly smooth, suggestive of an older stellar population.
