The galaxy presents as a moderately luminous object, exhibiting a slightly elongated morphology. A significant portion of the galaxy's light is concentrated in the central region, suggesting the presence of a prominent bulge or nucleus. While the galaxy appears mostly smooth, there is some visual indication of disturbed features, possibly due to a minor interaction or internal dynamics. There is a hint of bluer star forming regions, but the bulk of the galaxy shows a strong red/yellow tint, suggesting an older stellar population. 
