The galaxy presents a somewhat elongated morphology, appearing as a cigar shape in the image. The light is concentrated towards the center, suggesting a bulge component. There is evidence of an extended halo or disk surrounding the core. The galaxy exhibits a relatively smooth appearance, lacking the clear spiral arms or significant dust lanes characteristic of spiral galaxies. The color distribution appears relatively uniform, with a hint of redder hues. Overall, the galaxy appears to be a moderate mass system with very little ongoing star formation. There are no obvious signs of any strong interactions with other galaxies.
