This galaxy presents as an elliptical-like structure, generally smooth in appearance. Its central region exhibits a concentrated luminosity, which gradually decreases towards its outer edges. The galaxy displays an elongated shape, indicating a deviation from a perfectly circular form. There is a slight suggestion of a disturbance, possibly indicating a minor interaction or internal activity. The color profile shows a concentration of redder hues in the central bulge, suggesting an older stellar population. The outer regions display some bluer tones, possibly indicating pockets of more recent star formation, although the overall star formation rate appears to be relatively low. The galaxy does not show clear evidence of spiral arms or a prominent disk structure.
