The galaxy appears as a single, relatively smooth object with a slightly elongated, cigar-shaped morphology. There's a hint of a disk-like structure, but no distinct spiral arms or bar features are discernible in this image. The galaxy displays a relatively concentrated brightness profile, with a gradual decrease in luminosity from its center towards the edges. Its color profile suggests a population dominated by older stars, displaying a redder overall hue, indicating a subdued star formation rate. The galaxy does not show any major disturbances or signs of merging with another galaxy based on the smooth and largely undisturbed appearance. The object has an estimated effective radius of approximately 8.7 kpc and a stellar mass of approximately 10^10.9 solar masses, which makes it a medium sized galaxy.
