The galaxy presents as a generally smooth object, with a mildly elliptical shape. A bright central bulge is evident, grading outward into a less luminous, more diffuse halo. Color gradients indicate that the central region is yellower than the surrounding areas, suggesting an older stellar population within the bulge and possibly ongoing star formation in the outer regions. No obvious spiral arm structure or dust lanes are visible at this resolution. There is a very slight asymmetry in the outer halo, potentially indicating a minor interaction or disturbance. The galaxy's elongated shape suggests it is likely an elliptical galaxy.
