The galaxy appears as a relatively smooth, somewhat elliptical object. It has a slight elongation, but is closer to a circular morphology. There is no discernable disk structure and no apparent spiral arm features or bar. No significant dust lanes are visible. The galaxy seems to be composed of a fairly uniform distribution of light with a slight concentration toward the center, suggesting the presence of a bulge. The color seems to be a relatively uniform yellow, indicative of a population of older stars. No strong evidence of active star formation is apparent. There is no sign of major tidal disturbances or ongoing mergers, however, there may be some minor signs of gravitational disturbances. 
