The galaxy presents as a slightly elongated, cigar-shaped morphology. Its central bulge exhibits a bright, concentrated luminosity, indicating a significant population of older stars. The galaxy's disk appears relatively smooth and featureless, lacking prominent spiral arm structures. A faint blueish hue is visible at the outer edges of the disk, potentially indicating regions of more recent star formation. Overall, the galaxy appears relatively isolated and undisturbed, with no apparent signs of major tidal interactions or ongoing mergers.
