The galaxy presents as a relatively smooth, elongated structure, with a cigar-like shape. The core region exhibits a concentrated, bright, yellowish-white hue, suggesting a high density of older stellar populations. Progressing outward from the core, the luminosity gradually diminishes, transitioning to a faint blue-ish glow on the edges of the galaxy. There is no clear evidence of strong spiral arm structures or prominent dust lanes. The overall morphology appears undisturbed, with no indications of ongoing major mergers or significant tidal interactions. This galaxy likely represents a relatively massive system with a suppressed rate of star formation and a significant population of evolved stars.
