The galaxy presents as a somewhat elliptical structure with a noticeable bulge. The central region is bright, exhibiting a concentrated luminosity that gradually fades towards the outer edges of the galaxy. There is a subtle flattening of the galaxy along its minor axis, indicating some degree of ellipticity. While the overall structure appears relatively smooth, the galaxy may exhibit subtle features indicative of a disk component. The galaxy appears to be relatively isolated. The galaxy displays a relatively smooth texture without prominent spiral arms or other distinct features typically associated with spiral galaxies. The color profile is characterized by a warmer, reddish-yellow hue, particularly prominent in the central bulge, suggesting an older stellar population. 