The galaxy appears to be of relatively small angular size. It is generally elliptical in shape, but there are some noticeable irregularities. The galaxy's light profile seems to be composed of a dominant central region, surrounded by a slightly dimmer halo or extended disk. There is evidence of potential tidal features or disturbances, with slight, uneven extensions of light, particularly on one side. There appears to be a faint, somewhat blue-shifted region extending from the main body of the galaxy, which might suggest ongoing star formation in a disk like structure, or could be an artifact. Overall the galaxy appears to be interacting or possibly undergoing a merger event with another galaxy, but more data would be necessary to confirm. The distribution of light is non-uniform, with the central region appearing brighter.
