The galaxy presents as a relatively compact, elliptical object with a smooth and diffuse morphology. The light is concentrated centrally, showing a yellowish-white core, which suggests an older stellar population. There is an indication of some bluer, less concentrated light surrounding the central region, possibly indicating some star formation. The overall shape is mostly rounded, with hints of slight irregularities on the edges. There is no strong evidence of spiral arms or a defined disk structure. It does not appear to be undergoing any major merging activity.
