The galaxy presents an overall elliptical morphology, appearing relatively smooth with a concentrated central bulge. The color profile exhibits a gradient, transitioning from a brighter, more yellow-white core to a fainter, slightly reddish halo. There's little evidence of distinct spiral arm structures or significant dust lanes within the visible light spectrum. The galaxy's shape is close to round, with a minor ellipticity noticeable in its outer regions. There is no obvious evidence of ongoing major merger events, or tidal disturbances suggesting recent interactions. The overall color suggests a population dominated by older stars, indicative of a relatively low star formation rate. The galaxy displays a regular, undisturbed structure, indicating stability over a significant period.
