The galaxy appears as a somewhat smooth, elongated structure. It exhibits a concentrated central bulge that has a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy show a bluer tint, indicating the presence of younger stars. The galaxy's shape is more cigar-like rather than perfectly round. There is no strong evidence of any major ongoing merger events or significant tidal disturbances, although there appears to be a slight asymmetry that could indicate a minor interaction.
