This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light profile appears elliptical, tending towards a moderately rounded shape rather than a highly flattened disk or cigar-like form. There is no visually apparent evidence of spiral arm structure or strong tidal features indicating a major merger event. A minor disturbance or interaction cannot be entirely ruled out, but it is not prominently evident in the image. The galaxy presents a color gradient, with a central region displaying a yellowish hue, suggesting an older stellar population with lower ongoing star formation activity. The outer regions appear slightly bluer, though less prominent, potentially indicating a younger stellar population in the outer parts of the galaxy, or lower levels of star formation. Overall, the galaxy seems to be a relatively evolved system.
