The galaxy presents as a somewhat elliptical, extended object with a bright, concentrated central bulge. The color profile appears yellowish-white in the core, suggesting an older stellar population. There is evidence of a surrounding disk component, although it is not clearly defined. Faint blueish hues can be observed within the disk, possibly indicating regions of more recent star formation, though not significantly so.

The galaxy exhibits some indications of minor morphological disturbance or interaction, seen as asymmetry in the galaxy. 
