The galaxy presents a somewhat elongated, cigar-like morphology. Its light profile appears relatively smooth, with a central, brighter region that may indicate a higher concentration of stars, possibly a bulge. There is a hint of an extended structure, seen as a faint, diffuse glow extending outward from the main body, particularly at the bottom. This could be a very faint disk, tidal debris, or stellar halo. The color is predominantly yellowish-orange in the central region, suggesting an older stellar population. A slightly bluer component is potentially observable within this extended structure. There are no obvious signs of strong spiral arms or intense star-forming regions, indicating a more passive evolutionary state. There is little evidence of an active galactic nucleus from this image alone.
