The galaxy appears to be a luminous, early-type spiral galaxy with a notable bulge and a disk. The galaxy exhibits a generally smooth appearance, with a slight degree of elongation. The central bulge dominates the galaxy's light, appearing more concentrated and yellow in color, indicative of an older stellar population. A faint disk extends outwards, exhibiting a bluer hue compared to the bulge, suggesting the presence of younger, hotter stars and possible ongoing star formation. However, any spiral arm structure is indistinct. The galaxy's overall shape is primarily elongated but has slight roundness. There are no obvious signs of major interactions or mergers, although subtle disturbances can not be fully ruled out. Based on its red color it is likely a very massive galaxy with a low star formation rate and high metallicity.
