The galaxy presents as a moderately faint, elongated object. Its light is dominated by what appears to be an older stellar population, indicated by a color profile leaning towards the red end of the spectrum. There's no clear evidence of spiral arm structure or active star formation regions. The galaxy appears relatively smooth with a high degree of central concentration. The overall shape is more cigar-shaped than circular and shows no signs of ongoing merging activity, nor are there any significant tidal disturbances. The light is distributed quite evenly with a slight color gradient.
