The galaxy presents a predominantly smooth morphology. Its overall shape appears to be somewhat elliptical, leaning towards a cigar shape, with the major axis significantly longer than the minor axis. The light distribution is centrally concentrated, with the core exhibiting a bright, yellowish hue, indicative of an older stellar population. The outer regions display a fainter, greenish tint, suggesting the presence of some younger stars, though their overall contribution seems limited. There is no clear evidence of spiral arm structures or significant dust lanes within the visible portion of this galaxy. The galaxy does not show any signs of ongoing major mergers, though minor disturbances or interactions cannot be entirely ruled out based on this imagery alone.
