The galaxy presents a generally elliptical morphology, appearing elongated with a cigar-like shape. A prominent central bulge is observed, exhibiting a smooth, concentrated distribution of light, indicative of an older stellar population. The surrounding disk appears relatively smooth with hints of structure. There is some indication of a feature or disturbance in the disk with some slightly redder color, suggesting possible localized star formation or dust obscuration. Overall, the galaxy appears relatively isolated, with a low likelihood of undergoing any major merging events. The color profile suggests a moderate redshift.
