The galaxy presents as a moderately luminous object, exhibiting a predominantly smooth morphology with a slight elongation. The light distribution suggests an elliptical or lenticular form, where the bulge component appears dominant. There is a concentration of light towards the center, indicating a significant stellar density. The colors are indicative of a moderate redshift. A general lack of distinct spiral arm features or irregular structures suggests a relatively quiescent galaxy, possibly with limited ongoing star formation. There is a slightly noticeable change in color from the center to the edges of the galaxy, with the center of the bulge appearing to be a more yellow hue with the outer edges of the galaxy appearing to be more blue, hinting at a slightly younger stellar population on the outskirts of the galaxy. There is no evidence of significant tidal disturbances or ongoing major mergers.
