The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its morphology is largely featureless, with no apparent spiral arms or bar. The overall shape is somewhat flattened, appearing somewhere between round and elongated. A slight central bulge is present, exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter blue regions extend outward from the central area which may indicate some star forming regions, however the global star formation rate is observed to be low. There is some evidence of a minor gravitational disturbance, suggesting a possible past or ongoing interaction. The overall color suggests a mixture of stellar ages, with a dominant population of older, redder stars.
