The galaxy appears as an elliptical, somewhat lenticular structure, with a smooth, centrally concentrated luminosity profile. The nucleus is bright and possesses a yellowish hue, indicative of an older stellar population. Moving outwards from the core, there is a gradual decrease in surface brightness. There is a suggestion of a faint disk component, but the image resolution limits detailed assessment. The overall structure lacks distinct spiral arms or prominent dust lanes. The morphology seems relatively undisturbed, without obvious signs of major mergers or tidal interactions, however there is a hint of asymmetry. The galaxy exhibits a moderate redshift, implying a substantial distance and lookback time. The observed colors suggest ongoing, but relatively subdued, star formation.
