The galaxy presents as a relatively smooth, elliptical form, exhibiting a notable bulge in its central region. The light distribution is centrally concentrated, fading outwards. The main body of the galaxy appears yellow/orange, suggesting an older stellar population is dominant. The morphology is predominantly smooth, with some subtle, minor disturbances potentially observable in the outer regions. There is a possible secondary object close to the main galaxy, potentially in the form of a smaller satellite galaxy, however its proximity complicates definitive categorization. The primary galaxy does not appear to be undergoing a major merger.
