The galaxy presents as a flattened elliptical shape, elongated significantly along one axis, with an approximate aspect ratio of 2:1, tending towards a cigar shape. The central region exhibits a concentrated luminosity, appearing smooth and relatively featureless. The color profile suggests a population of older stars, with a yellow-orange hue dominating, indicating that the galaxy is in its red sequence. There is little to no evidence of spiral arm structure or prominent dust lanes. The galaxy appears undisturbed, with no obvious signs of recent or ongoing major mergers or tidal interactions. Faint color variations hint at subtle structural details, but high spatial resolution data is needed for further analysis. Overall, the galaxy appears to be a massive elliptical galaxy with minimal current star formation activity.
