The galaxy presents as a flattened spheroid with a relatively smooth texture. A bright, concentrated central bulge dominates the galaxy's overall luminosity profile. Surrounding the central region is a fainter, extended disk. The disk appears relatively featureless, showing no prominent spiral arm structures or dust lanes visible at this resolution. The galaxy exhibits a color gradient, transitioning from a whiter, bluer hue in the central bulge to a slightly redder color in the outer disk. This color difference could indicate variations in stellar populations and star formation activity across the galaxy, with the central bulge potentially hosting older, redder stars, and the outer disk showing evidence of younger, bluer stars. There might be minor disturbances or subtle asymmetries in the outer regions. Overall, the galaxy exhibits characteristics consistent with an intermediate or early-type spiral galaxy, or possibly a lenticular galaxy observed at an inclined angle relative to our line of sight.
