The galaxy presents a slightly disturbed morphology. A larger, more diffuse component shows a centrally concentrated light profile. Patches of bluer light suggest ongoing star formation. A secondary, smaller structure appears in close proximity, possibly indicating a minor interaction or tidal disturbance. The overall color is moderately blue, implying a mixed stellar population with a fraction of young, hot stars. The galaxy exhibits a moderately high degree of central concentration, though not perfectly spherical. There is no strong evidence of a major merger, although some asymmetry is noted.
