The galaxy presents as a somewhat elliptical, diffuse object. Its core region appears brighter and more concentrated, exhibiting a smooth, luminous profile. The galaxy's overall color appears to be slightly reddish, which could indicate an older stellar population and relatively low star formation activity. There is a suggestion of a faint, extended halo or envelope surrounding the main body of the galaxy, though the image resolution limits a detailed assessment of its structure and extent. The galaxy appears to be undergoing some type of interaction or disturbance, judging by the slight asymmetry present in its structure. It is elongated, but not greatly, and its structure looks mostly uniform without clear arm structures. The slight disturbance may be indicative of past merger activity.
