The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The overall shape approximates a circular form, with hints of a slight extension. There is some evidence of a disk-like structure, but it is not particularly well-defined. No obvious spiral arms or bar structures are discernible. The galaxy appears to be relatively isolated, with no major signs of recent merger activity, although minor disturbances cannot be ruled out. The galaxy possesses a redder color in its outer regions, potentially indicating a gradual change in stellar population towards older, redder stars away from the center.
