The galaxy presents as a relatively smooth, disk-like structure with a bright, concentrated central bulge. There is minimal evidence of spiral arm structure or prominent star-forming regions. The color profile suggests a population of older stars, indicated by the redder hue, particularly concentrated in the central bulge. Fainter blue light is also visible, potentially due to the existence of some young stars. Overall, this galaxy appears to be undergoing relatively low levels of star formation. There may be a slight asymmetry or irregularity in the disk, but it is not clear. There are no apparent signs of a major merger event or tidal interactions with other galaxies.
