This galaxy presents as a spiral or lenticular type, exhibiting a distinct central bulge that appears yellowish, suggesting an older stellar population within the core. The surrounding disk shows a bluer hue, potentially indicating the presence of younger stars and ongoing star formation. The disk does not seem to have clear spiral arm structure and could be described as flocculent. The overall shape appears somewhat elliptical and relatively smooth. The galaxy has a non-negligible inclination with respect to our line of sight. There is no visual evidence of any major mergers or tidal disturbances.