The galaxy presents a generally smooth appearance with a concentrated central bulge that dominates its overall structure. There appears to be a slight disk visible. The bulge exhibits a yellow-white hue, suggesting an older stellar population. The galaxy has a relatively round morphology, with only minor deviations from a perfect circular shape. Faint hints of a disk structure might be present but is difficult to confirm from the resolution of the data. The faint outer regions of the galaxy show evidence of a spiral pattern. There are no obvious signs of a major ongoing merger, although subtle irregularities in the galaxy's shape may indicate past interactions or minor disturbances. Based on the blueness in the disk, there appears to be only modest amounts of star formation occurring. The galaxy has a red shift of roughly 0.1, placing it at a substantial distance.
