The galaxy presents as a relatively compact structure, exhibiting a generally smooth morphology. There is a subtle, irregular distribution of light within the galaxy's body, hinting at underlying structures or ongoing processes. The overall shape appears somewhat elliptical, leaning towards round but not perfectly spherical. The galaxy presents a yellow-orange hue, with some red present, suggesting an older stellar population with potential regions of ongoing, but subdued, star formation. No prominent spiral arms or bar features are discernible. There is no apparent significant tidal distortion or signs of an ongoing major merger event. The galaxy could be undergoing a minor interaction, based on the slight irregularity.
