The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its shape is elongated, appearing as an ellipse rather than a perfect circle. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population. Surrounding this central bulge, there's a fainter, bluer disk-like structure. This bluer color could indicate more recent star formation activity within the disk. There may be some minor irregularities or asymmetries in the outer regions, though the image resolution makes it difficult to ascertain definitive merger events or tidal disturbances. The lack of distinct spiral arm structures supports its classification as an early-type spiral, a lenticular galaxy, or potentially an elliptical galaxy with some residual disk component. 
