This galaxy presents as a relatively symmetrical, elliptical form. It appears to be smooth and largely featureless, lacking prominent spiral arms or a distinct galactic bar. The central region exhibits a concentrated luminosity, suggesting a significant stellar density or possible active galactic nucleus. Moving outward, the galaxy's light gradually diminishes. There's a very slight bluing in the outer edges of the galaxy. The galaxy is reasonably round. It doesn't seem to be undergoing a major merger, although there might be minor disturbances within its structure that are not visible at this resolution. The color of the galaxy is in a range we might expect from older stellar populations. The galaxy appears to have significant mass, which implies a relatively large stellar population. The galaxy's star formation rate is in an average range.
