The galaxy presents as a relatively smooth, elliptical or lenticular structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-orange hue, potentially indicating an older stellar population. The galaxy lacks any prominent spiral arms or obvious dust lanes. There is a faint, diffuse halo surrounding the central region, gradually fading into the background sky. The overall shape is fairly round, with a possible slight elongation. No significant signs of recent or ongoing major mergers are apparent; however, a subtle asymmetry or minor distortion could be indicative of past gravitational interaction. The light profile suggests that the galaxy is relatively evolved, with limited ongoing star formation. The galaxy is of intermediate size for a galaxy at its given redshift.
