This galaxy presents as a smooth, elongated structure with a noticeable central bulge. The light distribution appears relatively uniform, transitioning gradually from the core to the outer edges. The color profile exhibits a bluer hue towards the center, indicative of possible ongoing or recent star formation activity. The galaxy lacks any prominent spiral arms or dust lanes, suggesting it is likely an elliptical or lenticular galaxy seen at an angle, possibly cigar shaped. There's no immediate visual evidence of any major mergers or significant tidal disturbances, although a minor disturbance can not be ruled out.
