The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a slight cigar shape. Its central region is characterized by a yellowish-orange hue, suggesting an older stellar population or a significant dust component. Fainter, bluish tinges are observed toward the outer edges of the galaxy, hinting at the presence of younger, hotter stars, but these are not prominent. There is no clear evidence of spiral arms or a defined disk structure, but it looks like there may be some ongoing low-level star formation. No major disturbances are visible in the galaxy's morphology, suggesting it is not currently undergoing a major merger.
