This galaxy presents as a somewhat elongated, cigar-shaped structure. The central region appears brighter and more concentrated, indicating a possible bulge. Fainter, diffuse light extends outwards from this central core, suggesting a disk component. The galaxy exhibits a relatively smooth appearance with no obvious spiral arm structures or significant dust lanes visible in this image. A slight blue tint is observable in the outer regions, possibly indicative of ongoing star formation, while the central regions appear more yellow. There are no immediately apparent signs of a major merger event, although subtle irregularities in the shape of the outer regions might indicate minor tidal disturbances or past interactions. Overall, the galaxy seems to be a relatively evolved system with a dominant spheroid component and a less prominent disk.
