The galaxy presents as a disk-shaped structure, viewed at a slight angle. A prominent central bulge is observed, contributing significantly to the galaxy's overall luminosity. The bulge appears relatively smooth. The disk component appears to show some faint, loosely defined spiral structures but they are not strongly contrasted. There isn't any clear evidence of on-going major merging events, or strong tidal disturbance features. The color distribution suggests a range of stellar populations. The center is redder suggesting older stars, which could mean that the star formation is somewhat suppressed, especially in the central regions. The outer disk is bluer in some spots, indicating the presence of younger, hotter stars, potentially indicating more recent or on-going star formation in these regions.
