The galaxy presents a generally smooth appearance with a concentrated central bulge, indicative of an elliptical or lenticular morphology. It displays a dominant yellowish-orange hue throughout the galaxy, suggesting an older stellar population with a relatively low rate of ongoing star formation. A subtle blue region is observed toward the upper left area of the galaxy, potentially indicating a region of recent or ongoing star formation. Subtle distortions are present in the galaxy's shape, possibly indicating tidal interactions with another galaxy or a past merger event.
