The galaxy presents a generally smooth morphology, with a noticeable lack of distinct features such as spiral arms or prominent dust lanes. It appears as a softly luminous, elliptical object. The galaxy's color profile exhibits a central concentration of yellow-orange hues, which could indicate an older stellar population dominating the core. Moving outward from the core, the color transitions to a bluer halo. The shape is best characterized as oblate. There is no evidence of strong tidal interactions or ongoing major mergers. The galaxy's integrated light suggests a moderate level of star formation activity. There are no obvious signs of dust obscuration.
