The galaxy appears to be an elliptical type, exhibiting a smooth, largely featureless morphology. It possesses a centrally concentrated luminosity profile, suggesting an older stellar population and a lack of significant ongoing star formation. The object displays a generally rounded form, with a slight elongation. There is an apparent interaction or close proximity with another object, which may be contributing to minor disturbances in the galaxy's overall structure. The lack of defined spiral arms or prominent dust lanes is consistent with this classification. Based on the colour profile, the system's stellar population likely consists predominantly of older, redder stars. Evidence of a potential merger or interaction with another galaxy is also indicated.
