The galaxy presents as a roughly elliptical or possibly a disk galaxy seen nearly face-on, displaying a notable central bulge. The galaxy's overall color appears to be slightly redder, especially towards the core, which might indicate an older stellar population and a lower rate of ongoing star formation. There is a faint hint of bluer light in the surrounding regions, possibly indicating some younger stars, and the overall luminosity suggests a galaxy with a stellar mass on the smaller side. No prominent spiral arms or bar structures are discernible in this image. There also appears to be little evidence of a recent or ongoing major merger, although there are minor features in the outer reaches of the galaxy which may suggest some disturbances. 
