The galaxy exhibits a generally smooth morphology with a slightly elongated, cigar-like shape. There is a dominant central bulge that appears relatively bright and diffuse, suggesting a high concentration of stars. The galaxy's overall color is slightly redder, which may indicate an older stellar population and a relatively low rate of ongoing star formation. Faint hints of spiral structure, or perhaps just irregularities in the light distribution, may be present, but they are not well-defined. No major signs of ongoing merging or significant tidal disturbances are readily apparent. It's possible the galaxy underwent a minor disturbance in the past.
