This galaxy exhibits an elongated morphology, appearing nearly edge-on from our vantage point. The central bulge is quite prominent and appears yellowish, indicating an older stellar population with reduced star formation. The galaxy displays a disk-like structure extending outwards from the bulge, also yellow, but to a lesser extent. There is evidence of a secondary concentration of light slightly above the central bulge, it is hard to tell if this is a satellite galaxy or a feature of the main galaxy. The galaxy does not appear to be undergoing major interactions, but some minor disturbances might be present based on its distorted shape. Overall, this galaxy appears to be a massive, evolved system, potentially with a relatively low rate of ongoing star formation.
