This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. There is little evidence of a prominent disk structure or spiral arms. The light distribution is concentrated towards the center, indicating a bright core, with the luminosity gradually decreasing outwards. The galaxy is dominated by older stellar populations, contributing to a redder color profile, although there are subtle hints of blue light indicative of a small population of younger, hotter stars. There is no clear indication of any major ongoing mergers, though a subtle asymmetry in the outer regions suggests the possibility of minor disturbances or past interactions. The overall structure is relatively undisturbed.
