The galaxy presents as a relatively smooth, elongated structure, suggesting an elliptical morphology. Its central region exhibits a concentrated, yellowish-white glow, indicating a high density of older stellar populations. Moving outward from the core, there is a transition to a fainter, bluish hue within the main body of the galaxy, possibly indicating more recent star formation in the outer regions. There is an absence of prominent spiral arms or distinct dust lanes. The galaxy appears to be isolated, showing no obvious signs of tidal interactions or ongoing mergers with other galaxies. A slight asymmetry might be present in its overall shape, but it does not clearly suggest any major disturbance.
