This galaxy presents as an elongated, cigar-shaped structure. It has a smooth, concentrated central bulge that appears yellowish in color, suggesting an older stellar population dominating the core. This central region gradually fades into a less concentrated, bluer disk. The disk exhibits a faint, diffuse structure with a slight tilt relative to our line of sight. No distinct spiral arms or prominent dust lanes are visible, which further supports the impression of a relatively smooth morphology. There is no obvious evidence of a major merger event or significant tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system, consistent with an elliptical or lenticular classification.
