The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests a possible elliptical galaxy, with a subtle deviation from a perfectly circular shape. There is a small central bulge or core that is brighter than the surrounding halo. The galaxy appears to have a smooth, diffuse envelope, lacking prominent spiral arms or strong dust lanes. There may be very slight asymmetry in its light distribution, but the overall structure appears undisturbed. The color suggests the presence of an older stellar population within the galaxy, though it cannot be determined with any certainty what the age of those stars might be. 
