The galaxy presents as an elongated, spindle-shaped structure indicative of an elliptical morphology, although some disk-like features appear to be present within the galactic structure. The central region exhibits a concentrated, bright, yellowish-white glow, suggesting a dense population of older stars. Fainter, bluish hues are visible extending from the central region, possibly indicating regions of more recent star formation within a galactic disk. There is no strong evidence of active galactic nuclei or significant dust lanes. The overall appearance indicates a relatively quiescent galaxy with moderate mass and a modest rate of star formation. There is no sign of recent merger activity or major disturbances of the galactic structure.