The galaxy presents as a slightly inclined disk galaxy. The central bulge region exhibits a bright, concentrated luminosity profile, suggestive of a significant stellar population. The disk component displays a bluer color, potentially indicating regions of active star formation, although the resolution limits a clear view of individual star-forming regions. There's a subtle hint of disturbance in the outer regions of the disk, possibly indicating a minor interaction or past merger event, however more information is needed for a definite assessment. The galaxy appears relatively isolated, with no immediately apparent major companion galaxies. There is some elongation.
