This galaxy presents a smooth, elongated morphology, likely an elliptical or lenticular type. The light distribution appears relatively uniform, with a bright central bulge that gradually fades towards the outer edges. The color profile indicates a predominantly older stellar population, exhibiting a redder hue at the core which transitions to bluer tones in the outer disk. The galaxy’s cigar-like shape may suggest an edge-on disk orientation and a low rate of ongoing star formation. There is no visible evidence of significant tidal disruption or interaction with neighboring galaxies. The galaxy's structure suggests it has a moderately low mass.
