This galaxy presents an elongated morphology, appearing somewhat cigar-shaped in its overall form. The light distribution seems relatively smooth, with a higher concentration of light towards the central region. There may be a subtle disruption in the structure, perhaps a minor tidal feature or faint arm-like extension, although the overall smoothness suggests a well-mixed stellar population. The color gradients across the galaxy are apparent; one end appears to be more blue-green while the opposite end is skewed towards a orange-red hue. This color gradient could indicate differences in stellar populations and/or dust content along the galaxy's length. The relatively red color in parts of the galaxy suggests the presence of older stars or significant dust obscuration. There is a possibility of an ongoing or recent minor merger event, though more high resolution imaging would be required to confirm this. The overall shape does not suggest a perfect elliptical galaxy, or a spiral galaxy.