The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light distribution appears relatively smooth across the major axis, showing a lack of strong spiral arm structure. There is a slight central bulge in the galaxy's central region, with the light smoothly decreasing towards the edges. The color is relatively uniform, with hints of redder hues suggesting an older stellar population. There is no significant evidence of ongoing major merging activity or strong tidal disturbances. The galaxy appears to be a relatively quiescent system.
