The galaxy presents as a somewhat elongated, cigar-shaped structure. It exhibits a relatively smooth morphology, with a central bulge that is brighter and more concentrated. The bulge appears to transition smoothly into a surrounding disk or halo. The overall color appears to be slightly redder, suggesting an older stellar population within the galaxy, though there is some evidence of bluer regions, possibly indicating ongoing, low-level star formation. There are no readily apparent spiral arms or significant dust lanes visible in the image. The galaxy does not seem to be undergoing any major merging events or significant tidal disturbances. 
