The galaxy appears to be a relatively smooth object, exhibiting a high degree of central concentration. It is moderately luminous, with a yellow-reddish hue indicative of an older stellar population and possibly significant dust extinction. There is a suggestion of a slightly elongated morphology, but the limited resolution prevents definitive classification. No spiral arm structures or prominent star-forming regions are discernible. The overall appearance suggests an elliptical or lenticular galaxy type, with limited ongoing star formation.
