The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a brighter, more concentrated luminosity. The light profile appears to gradually decrease in intensity outwards from this central bulge towards the edges of the galaxy. The overall shape could be classified as somewhere between elliptical and lenticular, leaning towards a cigar shape. While a defined disk structure is not readily apparent, there is a faint suggestion of a flattened component. There are some subtle asymmetries or minor disturbances visible, possibly indicative of past or ongoing gravitational interactions. The galaxy appears to be primarily emitting in the green and blue portions of the spectrum, perhaps indicating relatively high levels of star formation.
