The galaxy presents as a lenticular-like system exhibiting a notable disk component. The central bulge appears luminous, with a concentration of light suggesting an older stellar population. The disk is elongated, displaying an inclination relative to our line of sight. Dust lanes appear present, though not highly prominent, suggesting a relatively low dust content. The overall color profile indicates a mature galaxy, lacking the blue hues often associated with active star formation. The system appears relatively undisturbed, showing no strong evidence of ongoing mergers or tidal interactions. The galaxy exhibits a smooth appearance, lacking distinct spiral arms. The overall structure suggests a galaxy transitioning from a spiral to an elliptical morphology.
