This galaxy presents a predominantly smooth morphology, with an overall elliptical shape that is somewhat elongated, appearing more cigar-shaped than perfectly round. There is a subtle hint of disturbance in the galaxy’s form, potentially indicating a minor interaction or past merger event. The galaxy exhibits a color gradient, with a central region appearing bluer, possibly indicating the presence of younger, hotter stars, while the outer regions show a redder hue, which might suggest an older stellar population or a greater concentration of dust. The overall color suggests a relatively low rate of star formation. The galaxy doesn't appear to have well defined spiral arms or a prominent central bulge.
