The galaxy presents a flattened, elliptical morphology, viewed at an oblique angle relative to its major axis. The central region exhibits a high surface brightness, indicating a concentrated stellar population, likely an older population dominated by yellow and red light. There's a gradual decline in surface brightness towards the outer regions, though there's no clear or distinct spiral arm structure visible. There appears to be a slight bluing in the outer regions of the galaxy, indicating the presence of a young population of stars. Overall, the galaxy appears to be a relatively massive and evolved system, exhibiting characteristics intermediate between a pure elliptical and a spiral galaxy. There does not appear to be a presence of any tidal tails or disruptions to the galaxy.
