The galaxy presents as a relatively smooth, elliptical form with a noticeable central bulge. It appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The color profile suggests an older stellar population, with a yellowish-red hue concentrated within the central region, likely due to a higher density of evolved stars. A subtle color gradient exists, transitioning towards a slightly bluer periphery, which could indicate the presence of a younger, albeit less significant, stellar population in the outer regions. There is no obvious evidence of active galactic nucleus activity or ongoing major mergers. Faint tidal features cannot be ruled out, however, high resolution imaging may be required to detect them. The overall morphology is consistent with an early-type galaxy, possibly an elliptical galaxy with minimal ongoing star formation.
