The galaxy presents as a somewhat elliptical, yet relatively smooth object. The core exhibits a bright, concentrated luminosity, indicative of a high stellar density and potentially an active galactic nucleus. The overall color gradient transitions from a yellowish core to a redder, slightly fainter outer region, possibly suggestive of an older stellar population dominating the outer regions. There appears to be some distortion in the shape of the galaxy, possibly due to a minor interaction, though it is also possibly not, and may be a smooth galaxy. The isophotes, while not perfectly circular, do not present any prominent spiral arm structure or distinct morphological features. 
