The galaxy presents as a moderately luminous, somewhat elliptical structure. A concentrated central bulge region exhibits a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a diffuse disk, with bluer colors indicating the presence of younger, hotter stars. This disk appears relatively smooth with only subtle indications of spiral arms. Overall, the galaxy lacks prominent features or signs of active star formation. Based on visual morphology, it appears to be a relatively quiescent galaxy, likely an early-type spiral or lenticular galaxy, with a smooth light profile. There may be minor tidal disturbances as implied by morphological assessment. 
