The galaxy presents a distinctly elongated, cigar-shaped morphology, indicative of a classification leaning towards an elliptical type. Its structure appears primarily smooth, with a high concentration of light towards the central region, suggesting a prominent bulge. The color profile exhibits a yellow/red hue in the center, which could point towards an older stellar population and/or dust obscuration. Fainter blue regions appear on the very edge of the galaxy, possibly indicating areas of recent star formation, which are likely very minimal. There is no sign of spiral arms or a well-defined disk component. The galaxy displays no apparent signs of major mergers or significant tidal disturbances. Overall, the observed characteristics are consistent with an elliptical galaxy undergoing low levels of star formation.
