The galaxy presents as a slightly elongated, diffuse structure with a central bulge. It appears largely smooth, lacking the distinct spiral arm features often associated with disk galaxies. The galaxy's color profile suggests an older stellar population, with a yellow to reddish hue more pronounced towards the central bulge, indicating a concentration of evolved stars. There appears to be some bluer emission around the galaxy, possibly indicating star formation is occuring. It doesn't seem to be heavily distorted, nor are there any obvious signs of major interactions, though there could be minor disturbances present. 
