The galaxy presents as an elongated, cigar-shaped object, with a smooth appearance. The central region exhibits a concentrated, brighter luminosity suggesting a prominent galactic nucleus. Progressing outward from the core, the galaxy's luminosity gradually diminishes, forming a diffuse halo. A slight color gradient is observed; the central core appears yellowish, potentially indicating an older stellar population, while the outer regions exhibit a subtle shift towards reddish hues. There is no apparent indication of spiral arm structures or significant dust lanes, leading to a smooth, elliptical-like morphology. No distinct signs of ongoing major merging events are discernible. Slight asymmetry is present, possibly the result of a minor disturbance or interaction.
