The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a concentrated central bulge, which appears brighter and more uniform in color, transitioning gradually outwards. The galaxy's overall shape appears moderately elliptical, with a slight elongation. There is limited indication of distinct spiral arms or other significant disk features within the observed image. The galaxy has a red hue, suggesting older stellar populations and potentially lower rates of ongoing star formation. No indications of a major merger or significant tidal disturbances are evident, with the observed structure appearing relatively undisturbed. The galaxy's overall light profile indicates a fairly luminous system. The observed color gradient suggests some level of stellar population variation, with the inner regions potentially containing a higher concentration of older, redder stars, while the outer regions may contain slightly younger or bluer stars.
