The galaxy presents a somewhat elliptical morphology, appearing largely smooth in texture with a high degree of central concentration. A subtle color gradient is observed, with the central region exhibiting a yellowish-white hue, suggestive of an older stellar population. Fainter, bluish tinges are visible in the outer regions, potentially indicating ongoing or recent star formation, although these features are not particularly prominent. No distinct spiral arm structures or a well-defined disk component are discernible in this image. There appears to be a minor asymmetry to the morphology that could indicate a possible interaction with a smaller object or a remnant of a past merging event. Overall, the galaxy appears as a relatively compact system with a smooth light distribution and only subtle signs of recent star formation.
