The galaxy presents as an elliptical or lenticular morphology, with a predominantly smooth light distribution. The central bulge region appears brighter and more concentrated, exhibiting a yellowish hue, potentially indicative of an older stellar population. There is a discernible, though faint, halo surrounding the central region, which gradually fades into the background. No apparent spiral arm structures or dust lanes are visible. There is no clear evidence of ongoing major merging activity or significant tidal disturbances in this image. The overall shape appears generally round. 
