The galaxy presents an elliptical morphology with a generally smooth texture. The central region exhibits a higher luminosity, gradually decreasing towards the outer edges. There is a slight elongation visible, suggesting it is not perfectly spherical. The color profile shows a dominance of redder hues in the core, transitioning to bluer tones in the surrounding areas. This color variation might imply a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars distributed in the outer regions. There is subtle evidence of a possible minor disturbance or interaction, although the galaxy largely appears undisturbed, but these signs could use more in-depth observation.
