The galaxy presents as a lenticular, disk-shaped system, seen at an inclined angle relative to our line of sight. Its central region exhibits a concentrated, yellowish hue, suggestive of an older stellar population with minimal ongoing star formation. The outer regions show a bluer tinge, implying the presence of younger, hotter stars, though this component is significantly less prominent than the central bulge. Overall the galaxy appears generally smooth in texture, lacking distinct spiral arm structures or prominent dust lanes. The elongated shape indicates a rotating system, though without detailed spectroscopic analysis, the precise dynamics are difficult to ascertain. It displays characteristics of a galaxy in transition, possibly evolving from a spiral to an elliptical morphology.
