The galaxy presents as an elongated, cigar-shaped structure, suggesting it could be an elliptical galaxy viewed from the side or a highly inclined spiral. The central bulge appears prominent and concentrated, exhibiting a yellowish hue that implies an older stellar population. The outer regions of the galaxy are less defined, gradually fading into the background sky. A subtle disk-like structure may be present, though obscured by the inclination. The overall morphology indicates a relatively smooth structure with minimal signs of recent or ongoing major mergers or significant disturbances. Star formation appears to be low based on the color.
