The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The color profile suggests an older stellar population, as indicated by the dominant yellow-red hue, concentrated towards the center of the galaxy. There is a lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears to be quite compact, with a gradual fading of light intensity as it extends outwards from the central core. There is no clear evidence of ongoing major mergers or significant tidal disturbances within the visible structure of the galaxy, though subtle asymmetries might suggest minor interaction.
