The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a high degree of radial symmetry, with the intensity decreasing gradually from the center outwards. The dominant color is yellowish-orange, suggestive of an older stellar population with a lower rate of ongoing star formation. There may be a subtle, very faint hint of a disk structure, but it is not clearly defined. No distinct spiral arms, dust lanes, or active star-forming regions are readily apparent in the image. There appears to be little evidence of any ongoing major mergers or tidal disturbances.