The galaxy presents as a concentrated central bulge surrounded by a fainter, more diffuse disk. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The surrounding disk appears bluer, possibly indicating ongoing star formation, though this is not strongly evident from the image. The galaxy's overall shape is somewhat elongated, deviating slightly from a perfectly circular form. There is no clear indication of spiral arm structure or bar features within the disk. The galaxy appears relatively isolated, showing no obvious signs of interaction or tidal disturbances. It displays a generally smooth appearance, and its light distribution is consistent with an early-type spiral or lenticular galaxy morphology.
