The galaxy presents as a moderately bright, relatively small object, exhibiting a generally smooth, elliptical morphology. There is a slight elongation, but overall it appears quite rounded. No distinct spiral arms or bar structures are discernible. The galaxy's color is consistent with an older stellar population, appearing somewhat redder in comparison to other objects in the field, which could be due to redshift. No prominent signs of active galactic nuclei or substantial dust lanes are visible. The galaxy appears isolated, showing no clear evidence of ongoing major merging events or significant tidal disturbances from nearby companions. There may be minor disturbances, however it seems like there is little ongoing star formation.
