The galaxy presents as a centrally concentrated elliptical or lenticular-like system. It exhibits a largely smooth texture with no prominent spiral arm structures visible. The core region appears bright and somewhat unresolved, gradually fading into the outer regions. There is a slight elongation to the galaxy's overall shape, suggesting it is not perfectly spherical, instead approaching a more rounded morphology. A minor asymmetry or disturbance may be present in the form of a subtle extension on one side, but this is subtle. The galaxy appears to be a relatively quiescent system with a low star formation rate. There is no strong evidence of significant ongoing merger activity or major morphological disruption. The color profile shows a dominance of older stellar populations, with redder hues throughout, indicating minimal recent star formation.
