The galaxy presents as a centrally concentrated, luminous object with a roughly elliptical morphology. The core exhibits a bright, slightly blue-tinged glow, suggesting a region of enhanced stellar activity or a possible active galactic nucleus. The outer regions of the galaxy appear less defined, gradually fading into the background with a redder hue. There is a noticeable lack of spiral arm structures or distinct dust lanes, indicative of a smoother, potentially older stellar population. Faint irregularities or minor disturbances might be present in the outer halo, though the resolution makes definite characterization difficult. Overall, this galaxy appears to be an elliptical type.
