The galaxy exhibits a generally smooth morphology, with a predominantly elliptical shape. The light distribution appears concentrated toward the center, indicating a possible bulge component. The galaxy's color is predominantly yellow-white, suggestive of an older stellar population, but with a slight blue tint implying some recent star formation. A faint patch of yellower light is visible toward the edge of the galaxy, potentially indicating a region of different stellar population or dust distribution. There is no strong indication of spiral arms or a bar structure in the available image. It is not possible to determine if this is a merging galaxy from the image alone but there may be a minor disturbance.
