The galaxy presents as a relatively smooth, elongated structure, cigar shaped in appearance. It appears to be a disk galaxy, likely viewed edge-on or at a high inclination. The central bulge is visible, though not particularly prominent. There is some evidence of internal structure, but it is subtle, with a slightly mottled appearance rather than distinct spiral arms. Color variations are present, with a hint of bluer hues along the edges, which suggests the presence of younger stellar populations in the disk. The main body of the galaxy exhibits a redder color, indicating an older stellar population. There is no strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy seems to be a relatively isolated system, which is consistent with its classification as a fairly settled early type galaxy. There may be a smaller satellite galaxy in the bottom right corner.
