This galaxy exhibits a relatively smooth morphology, with a high concentration of light towards its center, suggesting a significant bulge component. The galaxy appears elongated, transitioning from a round to a more cigar-like shape. There are faint indications of a disk-like structure, but it is not prominently featured. The color profile suggests the presence of both older stellar populations, evident in the redder hues, and some younger, star-forming regions, as indicated by the bluer tints within the disk. No significant signs of ongoing merger activity or major tidal disturbances are apparent. Overall, the galaxy's features align with that of an early-type spiral or lenticular galaxy.
