The galaxy presents as a slightly elongated, moderately bright object. It exhibits a smooth, concentrated central bulge that dominates the overall light profile. There is little evidence of prominent spiral arm structure or significant dust lanes. The color appears to be predominantly blue-white in the central region, indicative of a younger stellar population. The outer regions of the galaxy display a faint, diffuse halo with a subtle color gradient towards redder hues, possibly suggestive of an older stellar population or the presence of dust. The overall morphology suggests an elliptical or lenticular galaxy type, with a near-absence of ongoing major star formation and no major disturbances or merging apparent in the image.
