The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a moderate degree of ellipticity, appearing nearly round but discernibly deviating from perfect circularity. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a bluer color, potentially indicating ongoing or recent star formation, though the resolution is insufficient to resolve individual star-forming regions. There is no clear evidence of spiral arm structure or a distinct disk component. No significant tidal features, or evidence of recent or ongoing major merger events are visible.
