The galaxy appears as a somewhat rounded, relatively smooth object with a dominant central bulge. The galaxy exhibits a yellow-red hue, indicative of an older stellar population and potentially lower levels of current star formation activity. There is a suggestion of a slight asymmetry or minor disturbance in the galaxy's morphology, possibly indicating a past or ongoing interaction with another galaxy, or an internal process affecting its structure. A faint, smaller, and somewhat distinct object is located close to the main galaxy, though it remains ambiguous whether this object is interacting with the primary galaxy or is simply another distant galaxy along the same line of sight. The main body of the galaxy demonstrates a high degree of central concentration.
