The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and spheroidal morphology with a high degree of central concentration. It has a distinct bulge component. There is a slight elongation present, indicating it is not perfectly spherical, but is closer to a spheroid than a disk. The color profile appears to be relatively uniform across the galaxy, with a yellowish-red hue suggestive of an older stellar population and potentially, relatively low levels of on-going star formation. There are no visually apparent spiral arms, dust lanes, or prominent star-forming regions. The galaxy exhibits a high degree of symmetry and does not display any clear signs of recent major mergers or tidal disturbances.
