This galaxy presents as a somewhat elongated, cigar-shaped object, indicating a possible elliptical morphology or a disk galaxy viewed at a high inclination angle. The central region exhibits a concentrated, bright core that appears yellowish-orange, suggesting an older stellar population. Fainter, bluish hues are seen towards the outer edges, potentially indicative of younger stars or ongoing star formation. There is no obvious spiral structure or prominent dust lanes, pointing to a lack of significant gas and dust content. Overall, the galaxy shows a relatively smooth and undisturbed appearance, with no apparent signs of recent major merging events, although minor tidal features or disturbances cannot be ruled out with the available resolution. The galaxy has an estimated radius of about 7.6 kpc.
