The galaxy presents as a luminous elliptical or lenticular system, exhibiting a predominantly smooth, centrally concentrated morphology. The main body displays a yellowish hue, suggestive of an older stellar population, with limited evidence of ongoing star formation within this region.  A notable feature is the presence of an apparent tidal tail or stream of material extending from the main galaxy body. This stream appears somewhat bluer in color, potentially indicating the presence of younger stars within this feature.  The overall form implies a potential recent or ongoing interaction or merger event contributing to the observed morphology and the presence of the extended stream.  The galaxy exhibits a relatively high degree of roundness, with only minor deviations from a perfectly elliptical shape, excluding the disturbance caused by the tail.
