This galaxy presents as a moderately luminous, elongated system. It appears to possess a dominant central bulge that is yellowish-orange in color, possibly indicating an older stellar population. Faint blue hues are present in the outer regions suggesting the presence of some younger, hotter stars and perhaps regions of ongoing star formation, though not particularly pronounced. The overall morphology is relatively smooth and lacks distinct spiral arm structures; the bulge dominates the overall form. The shape is highly elongated, and the light distribution appears symmetrical and undisturbed. There is no evidence of a major ongoing merger event, though there may be minor distortions suggesting a possible past interaction or minor disturbance. The galaxy has a moderate redshift, suggesting that it is fairly distant.
