The galaxy presents as a generally smooth structure, likely elliptical in nature given its form and lack of prominent spiral arms. A central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The galaxy's overall shape deviates slightly from perfectly circular, showing a somewhat elongated, though not excessively distorted, morphology. The outer regions display a fainter, bluish color, indicating the potential presence of younger, hotter stars. There may be a very slight disturbance in the morphology in the form of a faint extension or tidal feature, implying possible minor interactions with smaller galaxies or past merger events. Star formation activity appears low, if present at all, based on the limited blue light observed.
