The galaxy presents an overall elliptical morphology, appearing somewhat elongated. It exhibits a smooth light distribution, suggesting a lack of prominent spiral arms or distinct features. A bright, concentrated central bulge is evident, with the light intensity gradually decreasing towards the outer regions of the galaxy. There is some subtle color variation, shifting from a yellowish-white core towards a slightly redder hue in the outer regions. This color gradient might indicate differences in stellar populations, with older, redder stars dominating the outskirts. There's no obvious indication of recent or ongoing major mergers. However, there seems to be some slight asymmetry. Overall, the galaxy seems to be in a relatively evolved state, with a dominant population of older stars.
