The galaxy presents as a relatively smooth, elliptical morphology, with a concentrated central bulge. The light distribution appears fairly uniform without prominent spiral arms or significant dust lanes visible in this imaging. There is a slight elongation observed, deviating marginally from a perfectly circular shape. The galaxy exhibits a yellowish hue, suggesting a stellar population that is dominated by older, redder stars, with minimal ongoing star formation. There is no apparent interaction or merging activity with other galaxies in this image. Overall, the galaxy appears as a quiescent system.
