The galaxy presents as a centrally concentrated, ellipsoidal structure. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating this region. Moving outward from the core, the light becomes more diffuse with a gradual transition to a fainter, bluer color in the outer regions. This color gradient implies a possible distribution of younger, bluer stars within the galactic disk. The galaxy's overall morphology is relatively smooth. There is a lack of distinct spiral arm structures or prominent dust lanes that would indicate more active star formation. The shape is elongated, appearing more cigar-shaped than perfectly round. There appears to be a lack of any major merging signatures, with no obvious tidal tails or other significantly disturbed morphologies visible.
