The galaxy presents a primarily smooth morphology, suggesting it is an elliptical or lenticular galaxy. There's a slightly elongated shape, with an approximate aspect ratio of 0.8. The light is centrally concentrated with the brightest region at the core, gradually fading outwards, consistent with a de Vaucouleurs profile. The color distribution is not uniform, with the central region showing a yellower hue, possibly indicating an older stellar population with a smaller amount of star formation, transitioning to a bluer color further from the center, implying a population of younger, bluer stars in the outer regions. There are no obvious signs of spiral arms or a prominent disk structure and no strong evidence of recent major merger activity based on visual inspection. Overall the galaxy shows no significant disturbance.
