The galaxy presents a generally smooth morphology, exhibiting a dominant central bulge. There's very little evidence of spiral arms, although faint asymmetrical features suggest some possible faint disk or tidal disturbance. The galaxy is moderately elliptical.

The color profile appears to have a redder hue, potentially indicating an older stellar population, and relatively low rate of star formation within the galaxy. There is a concentration of light in the central region that gradually diffuses outwards with no clumpy star forming regions detected in the image. 
