The galaxy presents as an elongated, lenticular-like structure. Its core region exhibits a concentration of yellow-white light, indicative of an older stellar population. The surrounding regions are less concentrated, with a smoother gradient in luminosity. A slightly bluer hue is observed in the outer fringes of the galaxy, suggesting the presence of younger stars or ongoing star formation. There is no obvious spiral arm structure. The galaxy does not appear to be significantly disturbed or undergoing any major merger events. The shape is highly elongated, nearly cigar-shaped. Overall, this galaxy appears to be relatively smooth.
