The galaxy presents as a single, relatively smooth object with a slightly elliptical morphology. The central region exhibits a concentrated, bright yellowish-white core, suggesting a significant stellar population and potentially an active galactic nucleus. The galaxy's light appears to fade smoothly from the bright center towards the outer edges of the galaxy, without any obvious signs of spiral arms or distinct substructures. The color gradient from the core outward suggests a change in stellar populations, potentially indicating older, redder stars dominating the outer regions. There are no distinct tidal features or distortions evident, suggesting it has not recently undergone a major merger or interaction.
