The galaxy exhibits an elliptical morphology, appearing as a relatively smooth, concentrated distribution of light. The luminosity profile suggests a bulge-dominated system, with a gradual decline in surface brightness from the center outwards. A slight elongation is observed, indicating it is not perfectly spherical. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy's color appears somewhat red, indicative of an older stellar population, suggesting a lack of recent or ongoing major star formation activity. There appear to be no significant tidal features or distortions in the galactic structure, implying a quiescent merger history.
