The galaxy presents as a moderately bright, relatively smooth object. Its morphology appears to be predominantly elliptical, exhibiting a high degree of roundness with only subtle deviations from a perfect circular shape. No distinct spiral arms or a prominent central bar are apparent. The galaxy’s color profile suggests a predominantly older stellar population, exhibiting a reddish hue. There is some evidence of recent, weak star formation activity within the galaxy, as indicated by the bluer regions scattered throughout. The overall structure seems undisturbed, suggesting a lack of major mergers or significant tidal interactions in its recent past, though there may be some minor disturbances. The object is quite compact in size.
