The galaxy presents as a moderately luminous, disk-dominated system, exhibiting a subtle bulge at its center. The disk itself appears relatively smooth, with only hints of spiral arm structure visible. The light distribution within the disk is centrally concentrated, diminishing outwards towards the edges. The color profile suggests an older stellar population is present, with a slight reddening towards the central bulge, possibly indicating a higher concentration of dust or older stars in that region. There may be a low level of ongoing star formation. There is no obvious indication of strong tidal features or recent mergers. The overall appearance is consistent with a disk galaxy undergoing relatively quiescent evolution.
