The galaxy presents as a slightly elongated, elliptical-like structure. Its central region is characterized by a bright, concentrated luminosity suggesting a significant density of stars or an active galactic nucleus. The color of this central region appears yellowish-white. The light gradually fades outwards from the center toward the edges of the galaxy, where the color seems to shift towards a redder hue. The overall structure appears relatively smooth and lacks any prominent spiral arms, bars, or other distinct features associated with disk galaxies. There are no apparent signs of any major ongoing mergers or tidal disturbances, though some minor irregularities in the outer edges are possible at this resolution. Based on its shape, it may be an elliptical galaxy, but with a more cigar-like shape.