The galaxy exhibits a predominantly smooth morphology, with a concentrated central bulge. A faint, diffuse disk may be present, though its structure is not well-defined in this image. The galaxy appears to be moderately elliptical, not perfectly spherical. The light profile indicates a relatively high degree of central concentration. There are no prominent spiral arms or bar structures visible. The galaxy is redder in the center. The blue color around the edges of the galaxy may indicate some current star formation. No signs of major mergers or significant tidal disturbances are readily apparent. There are no visible dust lanes. The light is consistent with that of an older stellar population.
