The galaxy presents an elliptical morphology, exhibiting a smooth light distribution that diminishes gradually from the core outwards. It is characterized by a central bulge region that appears yellowish, indicating a likely older stellar population, with evidence of minimal recent star formation. The galaxy's disk appears relatively thin and is oriented at an angle, with the major axis extending horizontally in the image. The disk presents a subtle color gradient moving outwards from the core, suggesting a mixed population of older and intermediate-aged stars. The absence of clearly defined spiral arms or significant dust lanes supports its classification as an early-type galaxy.
