The galaxy presents as a slightly inclined, elongated system. Its morphology suggests a classification leaning toward a cigar shape. The central region appears relatively smooth, with a diffuse, yellowish glow, indicating an older stellar population. The outer regions appear less defined, showing a bluer tint, suggesting the presence of some younger stars, although star formation is not extensive. The overall light distribution is concentrated in the center, gradually fading outwards. There is no evidence of significant spiral arm structure or a prominent dust lane. The axial ratio suggests a moderately flattened structure. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances.
