The galaxy exhibits a bright, concentrated central bulge, indicating a high density of stars in its core. Surrounding the bulge is a more diffuse, elliptical-shaped halo with a relatively smooth texture. Faint hints of spiral arm structures may be present, although they are poorly defined and blended into the overall smooth appearance. The color profile appears to be fairly uniform across the galaxy, with a slightly redder hue indicative of older stellar populations. The overall morphology suggests an early-type spiral galaxy, perhaps transitioning into a lenticular galaxy due to the lack of prominent, well-defined spiral arms. There is no obvious evidence of recent mergers or significant tidal disturbances.
