The galaxy appears to be an elliptical galaxy with an elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated core, which gradually diffuses outwards into a fainter halo. The color gradient suggests an older stellar population, exhibiting redder hues concentrated towards the core with slightly bluer colors as one moves outwards from the center towards the edge of the galaxy. A subtle, but visible distortion is noted at one end of the galaxy, possibly indicating minor tidal interactions with a nearby object or internal dynamics. There does not appear to be any clear evidence of spiral arms or significant dust lanes within the main body of the galaxy.
