This galaxy, at a redshift of approximately 0.18, appears to be a relatively luminous system with an estimated effective radius of approximately 7 kpc. Morphologically, it is primarily smooth, with a slight elongation visible. There is a subtle suggestion of a disk-like structure, though the overall appearance is dominated by a centralized, smooth component. The galaxy exhibits a color gradient, with a bluer hue in its central region, transitioning to a redder color in the outer regions. This may indicate ongoing star formation in the core, with an older stellar population dominating the outer portions. The galaxy does not display obvious signs of major mergers or tidal disturbances, but some minor asymmetry cannot be ruled out. Overall, the morphology suggests a galaxy undergoing some level of quiescent evolution.
