The galaxy presents as a moderately bright, relatively smooth object with a noticeable elliptical morphology. The core exhibits a concentrated luminosity profile, suggesting a significant stellar population density. The main body of the galaxy displays a color gradient, transitioning from a redder hue at the central region to a bluer tinge in the outer regions. There is a very slight distortion of the galaxy disc, but it is relatively smooth. No obvious spiral arm structures or dust lanes are visible in this image. Overall, the galaxy is in a relatively relaxed state, without any ongoing major merger events or significant tidal disturbances apparent.
