The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge.  There is minimal discernible spiral structure or defined dust lanes. The color profile appears to be relatively homogenous, trending toward redder hues with a prominent yellowish core, suggestive of an older stellar population.  The galaxy's shape appears mostly round. There is no obvious evidence of major mergers or significant tidal disturbances. Faint hints of a disk may exist but cannot be definitively determined from the available image.
