The galaxy presents as a moderately bright, lenticular or early-type spiral system. It exhibits a relatively smooth, elliptical profile with a high degree of central concentration, suggesting a dominant bulge component. The light distribution shows a yellow-orange hue, indicative of an older stellar population, with a possible weak spiral structure component. Faint blue regions are present, implying some ongoing star formation. The galaxy appears slightly elongated, not perfectly circular, tending towards a "cigar" shape and there may be a slight hint of tidal disturbance or interaction.
