The galaxy presents as a small, elongated object with a discernible central bulge. The morphology suggests a likely elliptical or lenticular galaxy type, exhibiting a smooth light distribution with little evidence of spiral arms or active star formation regions. The galaxy appears somewhat cigar-shaped, with a significantly higher fraction of votes for it. A slight color gradient can be observed, transitioning from a blue hue at the outer edges to slightly redder tones near the central bulge. This suggests that the central regions may contain older stellar populations than the outer ones. There is no strong indication of merging events or tidal disturbances, though subtle asymmetries in the light distribution might suggest a possible minor interaction in its past. Based on the data provided, the galaxy is likely a relatively massive system, as it presents with very low levels of star formation.
