The galaxy presents as an elongated, cigar-shaped structure. Its luminosity appears concentrated toward the center, gradually decreasing outwards with no distinct edges. The color profile displays a generally redder hue towards the center and a slightly bluer tint to the outer regions. There is no visible spiral structure or other distinctive features like strong dust lanes or knots of star formation. It appears to be a relatively smooth distribution of light, possibly indicating that the system is an elliptical galaxy or a lenticular galaxy viewed edge-on. The low star formation rate may indicate an older stellar population. There is no apparent interaction with nearby companions or signs of ongoing merger activity.
