This galaxy presents as a centrally concentrated object with a smooth overall appearance, exhibiting characteristics leaning towards an elliptical morphology, although with some elongation suggestive of a potential disk or tidal disturbance. The light distribution is concentrated, transitioning from a bright, yellowish-white core to a fainter, bluish outer region. The relatively smooth light profile is minimally disturbed, with no obvious spiral arm structures or prominent dust lanes visible in this imaging. The colors suggest older stellar populations are dominant throughout the galaxy, though there may be some residual star formation taking place. There is some slight asymmetry to the light distribution, suggesting a possible minor interaction or past merger event.
