The galaxy presents an elongated, cigar-like morphology, indicating it is an elliptical galaxy viewed at an angle. The central bulge exhibits a yellowish hue, which is indicative of an older stellar population, with reduced star formation. The galaxy is relatively smooth in appearance, with little to no evidence of distinct spiral arms or significant dust lanes. A faint, bluish tinge is present in the outer regions, suggesting the presence of some younger, hotter stars, although star formation appears to be limited. There does not appear to be any major signs of a recent merger or interaction with another galaxy. Overall, the galaxy seems to be a relatively evolved system.
