This galaxy presents as a moderately inclined disk galaxy with a concentrated, bright central bulge. The disk shows evidence of some structural disturbance, exhibiting a slightly irregular morphology rather than a smooth, symmetric form. There are subtle hints of spiral arm structure, but they are not well-defined. The galaxy's color suggests a mix of stellar populations, with a bluer component indicative of younger stars, particularly within the disk region, and a redder component in the bulge, implying an older stellar population. There is some evidence of on-going star formation. Light emitted suggests it could possibly be undergoing a merger. The light from the galaxy spreads out about 3.5 arcsecs from the central point.
