The galaxy presents a distorted morphology, appearing elongated and potentially cigar-shaped. The light distribution within the galaxy appears uneven, with a brighter, more concentrated region at one end and a fainter, extended region at the other. There seems to be a smooth transition of luminosity in the center, with the edges being less luminous. The overall color of the galaxy appears to be somewhat yellow. This could indicate that the galaxy is composed of an older stellar population and exhibits a degree of dust extinction. The galaxy may be the result of a merger event, resulting in the disturbed morphology, or an interaction with another galaxy, which is not within the frame of the image. The morphology has a lack of spiral arms and lacks a prominent disk. There is some sign of potential tidal debris in the faint regions.
