The galaxy presents as a moderately bright, elliptical morphology. The central bulge appears dominant, with a high degree of sphericity. The light profile seems to smoothly decline from the nucleus outwards, showing no distinct features indicative of spiral arms or prominent dust lanes. The galaxy exhibits a slight elongation, but overall, it appears largely round. The color profile suggests a relatively passive stellar population, as the overall hue appears more yellow/red. There is no obvious evidence of ongoing major star formation activity, but a faint blue tinge hints at limited recent star formation in the outer disk. I do not see any signs of tidal distortions or ongoing mergers. There may be a very faint, diffuse halo, but it is difficult to discern due to the image quality.
