This galaxy appears to be an elongated, lenticular or possibly an elliptical type, seen edge-on or at a high inclination angle relative to our line of sight. The central bulge is prominent, with a yellowish-white color indicative of an older stellar population. Moving outwards from the center, the light gradually fades, suggesting a smooth distribution of stars and minimal dust obscuration. The galaxy exhibits a relatively smooth texture with no obvious spiral arms or distinct features. There are hints of faint blue light extending along the edges of the galaxy, possibly indicating some small amount of ongoing star formation. There does not appear to be any evidence of a major merger or tidal disturbances. Overall, this galaxy appears to be a relatively undisturbed system.
